Difference between revisions of "SHIPsProposal"
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** Why is this important? | ** Why is this important? | ||
** What is known, and not known? | ** What is known, and not known? | ||
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| + | {| class="wikitable" | ||
| + | |+Reading List | ||
| + | |- | ||
| + | ! scope="col"| Paper | ||
| + | ! scope="col"| Title | ||
| + | ! scope="col"| Description | ||
| + | ! scope="col"| Comments | ||
| + | ! scope="coI"| Assignment | ||
| + | |- | ||
| + | |[http://www.annualreviews.org/doi/abs/10.1146/annurev.astro.44.051905.092549?journalCode=astro Zinnecker & Yorke (2007) | ||
| + | |Toward Understanding Massive Star Formation | ||
| + | |Review article on massive star formation | ||
| + | |May need to get a free copy. | ||
| + | | | ||
| + | |- | ||
| + | |[http://adsabs.harvard.edu/abs/2008ApJS..179..249D Dunham et al. (2008)] | ||
| + | |Identifying the Low-Luminosity Population of Embedded Protostars in the c2d Observations of Clouds and Cores | ||
| + | | | ||
| + | | | ||
| + | | | ||
| + | |- | ||
| + | |[http://adsabs.harvard.edu/abs/2009ApJS..181..321E Evans et al. (2009)] | ||
| + | |The Spitzer c2d Legacy Results: Star-Formation Rates and Efficiencies; Evolution and Lifetimes | ||
| + | | | ||
| + | | | ||
| + | | | ||
| + | |} | ||
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* This work | * This work | ||
** What aspect of the "unknown" will we address in this work? | ** What aspect of the "unknown" will we address in this work? | ||
Revision as of 20:52, 7 February 2013
Contents
SHIPs Proposal
Abstract
A short, one or two paragraph, summary of the main points:
- What do we intend to do?
- Why is it important?
- How will we do it?
Science Introduction and Context
Topics to consider when writing this section.
- Background
- What is the scientific context of the work?
- Why is this important?
- What is known, and not known?
| Paper | Title | Description | Comments | Assignment |
|---|---|---|---|---|
| [http://www.annualreviews.org/doi/abs/10.1146/annurev.astro.44.051905.092549?journalCode=astro Zinnecker & Yorke (2007) | Toward Understanding Massive Star Formation | Review article on massive star formation | May need to get a free copy. | |
| Dunham et al. (2008) | Identifying the Low-Luminosity Population of Embedded Protostars in the c2d Observations of Clouds and Cores | |||
| Evans et al. (2009) | The Spitzer c2d Legacy Results: Star-Formation Rates and Efficiencies; Evolution and Lifetimes |
- This work
- What aspect of the "unknown" will we address in this work?
- Why is this interesting? How will it help?
- Target (An important part of carrying on the work).
- What target did we pick?
- Why this target?
- What is known in the literation?
| Paper | Title | Description | Comments | Assignment |
|---|---|---|---|---|
| Guetter & Turner (1997) | IC 1590, A Young Cluster Embedded in the Nebulosity of NGC 281 | |||
| Megeath & Wilson (1997) | The NGC 281 west cluster. I. Star formation in photoevaporating clumps. |
- What do we expect to find based on above?
- What Observations do we propose to do?
- What diagnostics will we use?
Analysis plan
Specifics about data and what to do with the data.
- How will the data be readied for this study? (Technical term: reduced, or processed).
- Ancillary data
- Where will we get our data?
- How will we supplement our data?
- How will we combine data?
- What tools will we use?
- To work with the data
- To produce the diagnostic plots.
Educational/Outreach plan
- The education angle for the general public.
- Implication for public education?
- Press release?
- Image release?
