Difference between revisions of "Jackie BRC 38"

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== Articles ==
 
== Articles ==
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| align="center" style="background:#f0f0f0;"|'''http://arxiv.org/pdf/1201.2704.pdf'''
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| align="center" style="background:#f0f0f0;"|'''URL'''
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| align="center" style="background:#f0f0f0;"|'''saurin 2012'''
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| align="center" style="background:#f0f0f0;"|'''Author Date'''
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| align="center" style="background:#f0f0f0;"|'''the embedded cluster or assoiciation trumpter 37 in ir 1396'''
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| align="center" style="background:#f0f0f0;"|'''Article Title'''
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| align="center" style="background:#f0f0f0;"|'''2MASS obsevations of BRC 38'''
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| align="center" style="background:#f0f0f0;"|'''Comments'''
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| http://arxiv.org/pdf/1201.2704.pdf||saurin et al. 2012  ||the embedded cluster or assoiciation trumpter 37 in ir 1396||2MASS obsevations of BRC 38  
 
|-
 
|-
 
| http://arxiv.org/pdf/1103.1646v1.pdf||Barensten et al.  2011||T tauri candidates and accretion rates using IPHAS: method and application to IC 1396||Includes BRC 38 which is called cloud E; Looking for YSOs in all of 1396; list 158 candidates; uses IPHAS survey data - Halpha, r, I filters on isaac newton telescope
 
| http://arxiv.org/pdf/1103.1646v1.pdf||Barensten et al.  2011||T tauri candidates and accretion rates using IPHAS: method and application to IC 1396||Includes BRC 38 which is called cloud E; Looking for YSOs in all of 1396; list 158 candidates; uses IPHAS survey data - Halpha, r, I filters on isaac newton telescope
 
|-
 
|-
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| http://arxiv.org/pdf/1005.1841v1.pdf||choudhury 2010||Triggered star formation and YSO population in Bright Rimmed SRO 38||44 YSOs identified in brc 38 - evidence for radiation driven implosion (RDI); spizter IRAC & MIPS data, optical BVRI
+
| http://arxiv.org/pdf/1005.1841v1.pdf||choudhury et al. 2010||Triggered star formation and YSO population in Bright Rimmed SRO 38||44 YSOs identified in brc 38 - evidence for radiation driven implosion (RDI); spizter IRAC & MIPS data, optical BVRI
 
|-
 
|-
 
| ||Morgan et al.  2010||Ammonia observations of bright-rimmed clouds: establishing a sample of triggered protostars||Radio observations (Green Bank) of brcs; furthering earlier work of morgan, confirming brc is triggered star formation site
 
| ||Morgan et al.  2010||Ammonia observations of bright-rimmed clouds: establishing a sample of triggered protostars||Radio observations (Green Bank) of brcs; furthering earlier work of morgan, confirming brc is triggered star formation site
 
|-
 
|-
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| http://arxiv.org/pdf/1005.0947v1.pdf||Crimier 2010||Physical structure of the envelopes of intermediate-mass protostars||a study that says that the mass of the final star of a protostar is linked to the mass of the envelope around the protostar, not the density of the parent cloud - backbground on IM protostars??
+
| http://arxiv.org/pdf/1005.0947v1.pdf||Crimier et al. 2010||Physical structure of the envelopes of intermediate-mass protostars||a study that says that the mass of the final star of a protostar is linked to the mass of the envelope around the protostar, not the density of the parent cloud - backbground on IM protostars??
 
|-
 
|-
 
| http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?2010ASInC...1...19O&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf||Ogura  2010||Triggered star formation assoicated with HII regions||Not really about BRC 38 but discusses curent state of triggered star formation theory
 
| http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?2010ASInC...1...19O&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf||Ogura  2010||Triggered star formation assoicated with HII regions||Not really about BRC 38 but discusses curent state of triggered star formation theory
Line 28: Line 31:
 
| http://arxiv.org/pdf/0902.4543v1.pdf||beltran et al.  2009||The stellar population and complex structure of the bright-rimmed cloud ic 1396N||A study through J< H< K\' filters; 736 sources found in all 3 bands (filters); h2 emission shows jet like structure
 
| http://arxiv.org/pdf/0902.4543v1.pdf||beltran et al.  2009||The stellar population and complex structure of the bright-rimmed cloud ic 1396N||A study through J< H< K\' filters; 736 sources found in all 3 bands (filters); h2 emission shows jet like structure
 
|-
 
|-
−
| http://cdsbib.u-strasbg.fr/cgi-bin/cdsbib?2009MNRAS.400.1726M||Morgan   2009||CO observations towards bright-rimmed clouds||can\'t get paper
+
| http://cdsbib.u-strasbg.fr/cgi-bin/cdsbib?2009MNRAS.400.1726M||Morgan et al.  2009||CO observations towards bright-rimmed clouds||can\'t get paper
 
|-
 
|-
−
| http://arxiv.org/pdf/0909.2267v1.pdf||fuente 2009||Dissecting an intermediate-mass (IM) prostar||A  look at IRAS 21391+5802 emissions of N2H+, CH3CN, CS, BIMA (1.2mm & 3.1mm)
+
| http://arxiv.org/pdf/0909.2267v1.pdf||fuente et al. 2009||Dissecting an intermediate-mass (IM) prostar||A  look at IRAS 21391+5802 emissions of N2H+, CH3CN, CS, BIMA (1.2mm & 3.1mm)
 
|-
 
|-
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| http://arxiv.org/pdf/0909.3312v1.pdf||Wang 2009||The relation between 13CO j=2-1 line width in moelcular clouds and bolometric luminosity of associated IRAS sources||IRAS 21391+5802 - suggests that it is a star forming cluster where high-mass stars will form
+
| http://arxiv.org/pdf/0909.3312v1.pdf||Wang et al. 2009||The relation between 13CO j=2-1 line width in moelcular clouds and bolometric luminosity of associated IRAS sources||IRAS 21391+5802 - suggests that it is a star forming cluster where high-mass stars will form
 
|-
 
|-
−
| http://arxiv.org/pdf/0903.2122v1.pdf||Chauhan 2009||Triggered star formation & evolution of t-tauri stars in and around BRC||Study that looked at ages of star forming clusters. Seems to be a lot of background materials on BRC 38
+
| http://arxiv.org/pdf/0903.2122v1.pdf||Chauhan et al. 2009||Triggered star formation & evolution of t-tauri stars in and around BRC||Study that looked at ages of star forming clusters. Seems to be a lot of background materials on BRC 38
 
|-
 
|-
−
| http://arxiv.org/pdf/0711.0775v1.pdf||Morgan 2007||A scuba survey of BRC||BRC 38 included in this study with SUBA data (submillimeter - microwave??); Classified as type B (tightly curved rims) which may be related to the strength of the ioisation field it is in
+
| http://arxiv.org/pdf/0711.0775v1.pdf||Morgan et al. 2007||A scuba survey of BRC||BRC 38 included in this study with SUBA data (submillimeter - microwave??); Classified as type B (tightly curved rims) which may be related to the strength of the ioisation field it is in
 
|-
 
|-
−
| http://arxiv.org/pdf/0705.2663v1.pdf||Neri 2007||The IC 1396N proto-cluster at a scale of ~250 AU||observations in millimeter range to help develop understanding of formation of clusters vs individual star formation
+
| http://arxiv.org/pdf/0705.2663v1.pdf||Neri et al. 2007||The IC 1396N proto-cluster at a scale of ~250 AU||observations in millimeter range to help develop understanding of formation of clusters vs individual star formation
 
|-
 
|-
−
| ||||||
+
| http://arxiv.org/pdf/astro-ph/0607006v2.pdf||Getman et al. 2007||X-ray study of triggered star formation and protostars in IC 1396N||x-ray sources in the globule of ic 1396N; good pictures to help with the visualization of 1396N and these sources; evidence of sequential star formation
 
|-
 
|-
−
| http://arxiv.org/pdf/astro-ph/0607006v2.pdf||Getman 2007||X-ray study of triggered star formation and protostars in IC 1396N||x-ray sources in the globule of ic 1396N; good pictures to help with the visualization of 1396N and these sources; evidence of sequential star formation
+
| http://arxiv.org/pdf/astro-ph/0702696v1.pdf||Patel et al. 2007||Submillimeter array observations of 321 ghz water maser emission in cepheus a||No don\'t think there is anything here
 
|-
 
|-
−
| http://arxiv.org/pdf/astro-ph/0702696v1.pdf||Patel  2007||Submillimeter array observations of 321 ghz water maser emission in cepheus a||No don\'t think there is anything here
+
| http://arxiv.org/pdf/astro-ph/0611634v1.pdf||Connelley et al. 2006||Infrared Nebulae around Young stellar objects||IRAS 21391+5802 - images show jet-like nebula and large patches of nebulosity
 
|-
 
|-
−
| http://arxiv.org/pdf/astro-ph/0611634v1.pdf||Connelley  2006||Infrared Nebulae around Young stellar objects||IRAS 21391+5802 - images show jet-like nebula and large patches of nebulosity
+
| http://arxiv.org/pdf/astro-ph/0508446v1.pdf||valdettaro et al. 2005||h2o maser emission from bright rimmed clouds in the northern hemisphere||H2O maser studied in brc 38; points to paper Valdettaro et al. 2005b
 
|-
 
|-
−
| http://arxiv.org/pdf/astro-ph/0508446v1.pdf||valdettaro  2005||h2o maser emission from bright rimmed clouds in the northern hemisphere||H2O maser studied in brc 38; points to paper Valdettaro et al. 2005b
+
| http://arxiv.org/pdf/astro-ph/0407102v1.pdf||Beltran et al. 2004||The dense moelcular cores in IRAS 21391 +5802 region||Three sources found with BIMA (??) observations in 21391+5802; Hard to read as they are trying to use data to fit/model how gas is emitted from the core
 
|-
 
|-
−
| http://arxiv.org/pdf/astro-ph/0407102v1.pdf||Beltran  2004||The dense moelcular cores in IRAS 21391 +5802 region||Three sources found with BIMA (??) observations in 21391+5802; Hard to read as they are trying to use data to fit/model how gas is emitted from the core
+
| http://iopscience.iop.org/1538-4357/593/1/L47/pdf/17405.web.pdf||Reipurth et al. 2003||Blowout from IC 1396N: The emergence of Herbig-Haro flows from a cloud core||Herbig-Haro flow (HH 777) found coming out of ic 1396N; located at 214041.6+581638 (in IR, I think)
−
|-
 
−
| http://iopscience.iop.org/1538-4357/593/1/L47/pdf/17405.web.pdf||Reipurth 2003||Blowout from IC 1396N: The emergence of Herbig-Haro flows from a cloud core||Herbig-Haro flow (HH 777) found coming out of ic 1396N; located at 214041.6+581638 (in IR, I think)
 
 
|-
 
|-
 
| http://adsabs.harvard.edu/full/2002aprm.conf..191O||Ogura, et el  2002||A large number of Halpha emission stars and Herbig-Haro objects in and around BRC||short (2 pages) listing observations of halpha emission stars - brc 38 has 7
 
| http://adsabs.harvard.edu/full/2002aprm.conf..191O||Ogura, et el  2002||A large number of Halpha emission stars and Herbig-Haro objects in and around BRC||short (2 pages) listing observations of halpha emission stars - brc 38 has 7
Line 58: Line 59:
 
| http://arxiv.org/pdf/astro-ph/0203206v1.pdf||Beltran  et al. 2002||IRAS 21391+5802: The Molecular Outflow and its Exciting source||VLA and BIMA observations of dust and gas surrounding IRAS source; 3 sources isolated with BIMA, each a YSO
 
| http://arxiv.org/pdf/astro-ph/0203206v1.pdf||Beltran  et al. 2002||IRAS 21391+5802: The Molecular Outflow and its Exciting source||VLA and BIMA observations of dust and gas surrounding IRAS source; 3 sources isolated with BIMA, each a YSO
 
|-
 
|-
−
| http://www.aanda.org/index.php?option=com_article&access=bibcode&Itemid=129&bibcode=2001A%26A...376..271CFUL||Codella  2001||Star formation in the BRC of IC 1396N||The density of several different molecular outflows (dense areas of particular molecules)in the globule looked at with 30m IRAM and OVRO interferometer. Demonstrates this area very complex.  
+
| http://www.aanda.org/index.php?option=com_article&access=bibcode&Itemid=129&bibcode=2001A%26A...376..271CFUL||Codella et al. 2001||Star formation in the BRC of IC 1396N||The density of several different molecular outflows (dense areas of particular molecules)in the globule looked at with 30m IRAM and OVRO interferometer. Demonstrates this area very complex.  
 
|-
 
|-
−
| http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?2001A%26A...376..553N&db_key=AST&nosetcookie=1||Nisini 2001||Multiple H2 protostellar jets in the bright-rimmed globule IC 1396-N||1st detection of H2 jets from YSO. Are these HH objects?  
+
| http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?2001A%26A...376..553N&db_key=AST&nosetcookie=1||Nisini et al. 2001||Multiple H2 protostellar jets in the bright-rimmed globule IC 1396-N||1st detection of H2 jets from YSO. Are these HH objects?  
 
|-
 
|-
−
| http://iopscience.iop.org/0004-637X/526/1/236/pdf/39770.web.pdf||Slysh 1999||Prootoplanetary disk and/or bipolar outflow traced by h2o masers in ic 1396n||Description of 3 models that may explain how masers form; Gives background on IC 1396
+
| http://iopscience.iop.org/0004-637X/526/1/236/pdf/39770.web.pdf||Slysh et al. 1999||Prootoplanetary disk and/or bipolar outflow traced by h2o masers in ic 1396n||Description of 3 models that may explain how masers form; Gives background on IC 1396
 
|-
 
|-
 
| http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1999sf99.proc..381O&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf||Ogura & Sugitani  1999||A large number of Halpha Emission Stars associated with BRCs||Supports \"small-scale sequential star formation\"; suggests low-mass stars formating in area of high-mass star forming area
 
| http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1999sf99.proc..381O&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf||Ogura & Sugitani  1999||A large number of Halpha Emission Stars associated with BRCs||Supports \"small-scale sequential star formation\"; suggests low-mass stars formating in area of high-mass star forming area
Line 68: Line 69:
 
| http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1999sf99.proc..358S&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf||Sugitani et al.  1999||Small-Scale Sequential Star Formtion in Bright-Rimmed Clouds||Discussion of small-scale sequential star formation hypothesis
 
| http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1999sf99.proc..358S&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf||Sugitani et al.  1999||Small-Scale Sequential Star Formtion in Bright-Rimmed Clouds||Discussion of small-scale sequential star formation hypothesis
 
|-
 
|-
−
| http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1996A%26A...315L.293S&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf||Saraceno 1996||LWS observations of the bright-rimmed globule IC 1396N||spectrum of co, oh, h2o are detected in the ISO-LWS spectrum - not sure what that is??
+
| http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1996A%26A...315L.293S&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf||Saraceno et al. 1996||LWS observations of the bright-rimmed globule IC 1396N||spectrum of co, oh, h2o are detected in the ISO-LWS spectrum - not sure what that is??
 
|-
 
|-
−
| http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1996A%26A...309..827S&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf||Saraceno 1996||An evolutionary diagram for young stellar objects||background - but not sure I understand it
+
| http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1996A%26A...309..827S&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf||Saraceno et al. 1996||An evolutionary diagram for young stellar objects||background - but not sure I understand it
 
|-
 
|-
 
| http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1996A%26A...309..581W&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf||Weikard et al.  1996||the structure of the IC 1396 region||Discussion of structure of 1c 1396 and the central star O6.5 (HD 206267) radiation on clumping and structure/location of yso; shows locations of yso in brc 38 from their data
 
| http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1996A%26A...309..581W&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf||Weikard et al.  1996||the structure of the IC 1396 region||Discussion of structure of 1c 1396 and the central star O6.5 (HD 206267) radiation on clumping and structure/location of yso; shows locations of yso in brc 38 from their data
 
|-
 
|-
−
| http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1991ApJS...77...59S&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf||Sugitani 1991||A catalog of BRC with iras point sources||Just a list of point sources they invesigated - brc 38 on the list
+
| http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1991ApJS...77...59S&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf||Sugitani et al. 1991||A catalog of BRC with iras point sources||Just a list of point sources they invesigated - brc 38 on the list
 
|-
 
|-
 
| http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1989ApJ...342L..87S&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf||Sugitani et al. 1989||Star formation in bright-rimmed globules: evidence for radiation-driven implosion||Argument for rdiation-driven implosion method of star formation.
 
| http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1989ApJ...342L..87S&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf||Sugitani et al. 1989||Star formation in bright-rimmed globules: evidence for radiation-driven implosion||Argument for rdiation-driven implosion method of star formation.
 
|-
 
|-
−
| http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1956BAN....13...77P&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf||Pottasch 1956||a study of bright rims in diffuse nebulae||Early work describing the location, shape of, density of, brightness of bright rim clouds in several nebula, including IC 1396 and Brc 38
+
| http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1956BAN....13...77P&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf||Pottasch et al. 1956||a study of bright rims in diffuse nebulae||Early work describing the location, shape of, density of, brightness of bright rim clouds in several nebula, including IC 1396 and Brc 38
 +
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 +
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Revision as of 22:06, 13 February 2012

Information about BRC 38

Search phrases

  • BRC 38
  • sfo 38
  • 21:40:42+52:16:13
  • 21391+5802
  • IC 1396N
  • Cepheus OB2

Articles

URL Author Date Article Title Comments
http://arxiv.org/pdf/1201.2704.pdf saurin et al. 2012 the embedded cluster or assoiciation trumpter 37 in ir 1396 2MASS obsevations of BRC 38
http://arxiv.org/pdf/1103.1646v1.pdf Barensten et al. 2011 T tauri candidates and accretion rates using IPHAS: method and application to IC 1396 Includes BRC 38 which is called cloud E; Looking for YSOs in all of 1396; list 158 candidates; uses IPHAS survey data - Halpha, r, I filters on isaac newton telescope
http://arxiv.org/pdf/1005.1841v1.pdf choudhury et al. 2010 Triggered star formation and YSO population in Bright Rimmed SRO 38 44 YSOs identified in brc 38 - evidence for radiation driven implosion (RDI); spizter IRAC & MIPS data, optical BVRI
Morgan et al. 2010 Ammonia observations of bright-rimmed clouds: establishing a sample of triggered protostars Radio observations (Green Bank) of brcs; furthering earlier work of morgan, confirming brc is triggered star formation site
http://arxiv.org/pdf/1005.0947v1.pdf Crimier et al. 2010 Physical structure of the envelopes of intermediate-mass protostars a study that says that the mass of the final star of a protostar is linked to the mass of the envelope around the protostar, not the density of the parent cloud - backbground on IM protostars??
http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?2010ASInC...1...19O&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf Ogura 2010 Triggered star formation assoicated with HII regions Not really about BRC 38 but discusses curent state of triggered star formation theory
http://arxiv.org/pdf/0902.4543v1.pdf beltran et al. 2009 The stellar population and complex structure of the bright-rimmed cloud ic 1396N A study through J< H< K\' filters; 736 sources found in all 3 bands (filters); h2 emission shows jet like structure
http://cdsbib.u-strasbg.fr/cgi-bin/cdsbib?2009MNRAS.400.1726M Morgan et al. 2009 CO observations towards bright-rimmed clouds can\'t get paper
http://arxiv.org/pdf/0909.2267v1.pdf fuente et al. 2009 Dissecting an intermediate-mass (IM) prostar A look at IRAS 21391+5802 emissions of N2H+, CH3CN, CS, BIMA (1.2mm & 3.1mm)
http://arxiv.org/pdf/0909.3312v1.pdf Wang et al. 2009 The relation between 13CO j=2-1 line width in moelcular clouds and bolometric luminosity of associated IRAS sources IRAS 21391+5802 - suggests that it is a star forming cluster where high-mass stars will form
http://arxiv.org/pdf/0903.2122v1.pdf Chauhan et al. 2009 Triggered star formation & evolution of t-tauri stars in and around BRC Study that looked at ages of star forming clusters. Seems to be a lot of background materials on BRC 38
http://arxiv.org/pdf/0711.0775v1.pdf Morgan et al. 2007 A scuba survey of BRC BRC 38 included in this study with SUBA data (submillimeter - microwave??); Classified as type B (tightly curved rims) which may be related to the strength of the ioisation field it is in
http://arxiv.org/pdf/0705.2663v1.pdf Neri et al. 2007 The IC 1396N proto-cluster at a scale of ~250 AU observations in millimeter range to help develop understanding of formation of clusters vs individual star formation
http://arxiv.org/pdf/astro-ph/0607006v2.pdf Getman et al. 2007 X-ray study of triggered star formation and protostars in IC 1396N x-ray sources in the globule of ic 1396N; good pictures to help with the visualization of 1396N and these sources; evidence of sequential star formation
http://arxiv.org/pdf/astro-ph/0702696v1.pdf Patel et al. 2007 Submillimeter array observations of 321 ghz water maser emission in cepheus a No don\'t think there is anything here
http://arxiv.org/pdf/astro-ph/0611634v1.pdf Connelley et al. 2006 Infrared Nebulae around Young stellar objects IRAS 21391+5802 - images show jet-like nebula and large patches of nebulosity
http://arxiv.org/pdf/astro-ph/0508446v1.pdf valdettaro et al. 2005 h2o maser emission from bright rimmed clouds in the northern hemisphere H2O maser studied in brc 38; points to paper Valdettaro et al. 2005b
http://arxiv.org/pdf/astro-ph/0407102v1.pdf Beltran et al. 2004 The dense moelcular cores in IRAS 21391 +5802 region Three sources found with BIMA (??) observations in 21391+5802; Hard to read as they are trying to use data to fit/model how gas is emitted from the core
http://iopscience.iop.org/1538-4357/593/1/L47/pdf/17405.web.pdf Reipurth et al. 2003 Blowout from IC 1396N: The emergence of Herbig-Haro flows from a cloud core Herbig-Haro flow (HH 777) found coming out of ic 1396N; located at 214041.6+581638 (in IR, I think)
http://adsabs.harvard.edu/full/2002aprm.conf..191O Ogura, et el 2002 A large number of Halpha emission stars and Herbig-Haro objects in and around BRC short (2 pages) listing observations of halpha emission stars - brc 38 has 7
http://arxiv.org/pdf/astro-ph/0203206v1.pdf Beltran et al. 2002 IRAS 21391+5802: The Molecular Outflow and its Exciting source VLA and BIMA observations of dust and gas surrounding IRAS source; 3 sources isolated with BIMA, each a YSO
http://www.aanda.org/index.php?option=com_article&access=bibcode&Itemid=129&bibcode=2001A%26A...376..271CFUL Codella et al. 2001 Star formation in the BRC of IC 1396N The density of several different molecular outflows (dense areas of particular molecules)in the globule looked at with 30m IRAM and OVRO interferometer. Demonstrates this area very complex.
http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?2001A%26A...376..553N&db_key=AST&nosetcookie=1 Nisini et al. 2001 Multiple H2 protostellar jets in the bright-rimmed globule IC 1396-N 1st detection of H2 jets from YSO. Are these HH objects?
http://iopscience.iop.org/0004-637X/526/1/236/pdf/39770.web.pdf Slysh et al. 1999 Prootoplanetary disk and/or bipolar outflow traced by h2o masers in ic 1396n Description of 3 models that may explain how masers form; Gives background on IC 1396
http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1999sf99.proc..381O&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf Ogura & Sugitani 1999 A large number of Halpha Emission Stars associated with BRCs Supports \"small-scale sequential star formation\"; suggests low-mass stars formating in area of high-mass star forming area
http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1999sf99.proc..358S&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf Sugitani et al. 1999 Small-Scale Sequential Star Formtion in Bright-Rimmed Clouds Discussion of small-scale sequential star formation hypothesis
http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1996A%26A...315L.293S&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf Saraceno et al. 1996 LWS observations of the bright-rimmed globule IC 1396N spectrum of co, oh, h2o are detected in the ISO-LWS spectrum - not sure what that is??
http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1996A%26A...309..827S&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf Saraceno et al. 1996 An evolutionary diagram for young stellar objects background - but not sure I understand it
http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1996A%26A...309..581W&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf Weikard et al. 1996 the structure of the IC 1396 region Discussion of structure of 1c 1396 and the central star O6.5 (HD 206267) radiation on clumping and structure/location of yso; shows locations of yso in brc 38 from their data
http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1991ApJS...77...59S&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf Sugitani et al. 1991 A catalog of BRC with iras point sources Just a list of point sources they invesigated - brc 38 on the list
http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1989ApJ...342L..87S&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf Sugitani et al. 1989 Star formation in bright-rimmed globules: evidence for radiation-driven implosion Argument for rdiation-driven implosion method of star formation.
http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1956BAN....13...77P&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf Pottasch et al. 1956 a study of bright rims in diffuse nebulae Early work describing the location, shape of, density of, brightness of bright rim clouds in several nebula, including IC 1396 and Brc 38
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