SFO Paper Journals Guided Reading - Revision history

Novatne: /* Info to help you answer questions and things I just don't get */

2012-05-06T16:16:36Z

Info to help you answer questions and things I just don't get

Piper at 17:47, 30 April 2012

2012-04-30T17:47:38Z

Piper at 17:46, 30 April 2012

2012-04-30T17:46:46Z

Piper at 01:34, 28 April 2012

2012-04-28T01:34:52Z

Piper at 01:21, 28 April 2012

2012-04-28T01:21:27Z

Piper at 22:59, 27 April 2012

2012-04-27T22:59:53Z

Piper at 22:58, 27 April 2012

2012-04-27T22:58:03Z

Piper at 19:22, 27 April 2012

2012-04-27T19:22:09Z

Piper: Created page with "=SFO Paper Journals Guided Reading= ==Original SFO - Sugitani et al 1991== Survey of BRCs to describe the BRCs themselves and look for YSOs.

Palomar Sky Survey (P..."

2012-04-27T19:13:16Z

Created page with "=SFO Paper Journals Guided Reading= ==Original SFO - Sugitani et al 1991== Survey of BRCs to describe the BRCs themselves and look for YSOs. Palomar Sky Survey (P..."

New page

=SFO Paper Journals Guided Reading=

==Original SFO - Sugitani et al 1991==
Survey of BRCs to describe the BRCs themselves and look for YSOs. 
Palomar Sky Survey (PSS) and IRAS point sources. 

44 BRCs found in Palomar Sky survey prints that had associated IRAS point sources where all found to have IRAS point sources that were good candidates for being YSOs. Tables/images exist for; HII region locations, PPS finding charts, BRC location charts, IRAS point source properties (12, 25, 60, 100 micron), BRC and point source descriptions and plots. 

Questions to ask yourself as you read 

Abstract, Intro and Summary 
-what is the flow of all the types of nebulosity that they describe and the cause/effect relationship to star formation? 
-how will the understanding of this cause/effect help us in our closer study of just three BRCs? 

The Sample, Results 
-how did the authors take advantage of Palomar Sky Survey Prints? 
-how will this help future astronomers with their work? 
-table 3 lists exactly one IRAS source for each BRC, where are the rest of the YSOs we expect to see? 
Discussion 
Although 15 of the IRAS point sources were catagoized as type I and “really are” YSOs, why are all 44 of the sources considered good candidates for YSOs?

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 Introduction, Observations and Data Reduction<BR>
--why do the authors recommend higher resolution studies?
+-why do the authors recommend higher resolution studies?<BR>
 -what is SSSSF and what is the evidence for supporting this hypothesis?<BR>
 -what is grism spectroscopy and how does it help “fill in some holes” in terms of YSOs?<BR>

@@ Line 29: / Line 29: @@
 Introduction, Observations and Data Reduction<BR>
 -what is SSSSF and what is the evidence for supporting this hypothesis?<BR>
 -what is grism spectroscopy and how does it help “fill in some holes” in terms of YSOs?<BR>

← Older revision		Revision as of 01:34, 28 April 2012
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−	=[[Info to help you answer questions and things I just don't get]]=	+	==[[Info to help you answer questions and things I just don't get]]==

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 ==Original SFO - Sugitani et al 1991==
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 Looking for H-alpha emissions using grism spectroscopy to find previously undetected YSOs that do not have strong IR excess in order to collect more information on star formation in BRCs and contained HH objects, and further investigate small-scale sequential star formation (SSSSF). <BR><BR>
 Optical (H-alpha using grism spectroscopy), 2 MASS<BR><BR>
 Questions to ask yourself as you read<BR><BR>
 Introduction<BR>
 -what is SSSSF and what is the evidence for supporting this hypothesis?<BR>
--what is grism spectroscopy and how does it help “fill in some holes” in terms of YSOs?<BR><BR>
+-what is grism spectroscopy and how does it help “fill in some holes” in terms of YSOs?<BR>
 Images and Data<BR>
 -what qualitative and quantitative information will be helpful to us in our study?  List tables and images, highlighting information specific to our study.<BR><BR>

@@ Line 24: / Line 24: @@
 Optical (H-alpha using grism spectroscopy), 2 MASS<BR><BR>
 Questions to ask yourself as you read<BR><BR>
-Introduction<BR><BR>
+Introduction<BR>
--what is SSSSF and what is the evidence for supporting this hypothesis?<BR><BR>
+-what is SSSSF and what is the evidence for supporting this hypothesis?<BR>
 -what is grism spectroscopy and how does it help “fill in some holes” in terms of YSOs?<BR><BR>
-Images and Data<BR><BR>
+Images and Data<BR>
 -what qualitative and quantitative information will be helpful to us in our study?  List tables and images, highlighting information specific to our study.<BR><BR>
-H-alpha stars, HH objects and Discussion<BR><BR>
+H-alpha stars, HH objects and Discussion<BR>
--what did the authors find of interest in our particular BRCs?<BR><BR>
+-what did the authors find of interest in our particular BRCs?<BR>
 -what evidence is given to support further multi-wavelength studies searching for YSOs?