Difference between revisions of "SHIPsProposal"
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|[http://adsabs.harvard.edu/abs/1998ASPC..148..150E Elmegreen (1998)] | |[http://adsabs.harvard.edu/abs/1998ASPC..148..150E Elmegreen (1998)] | ||
|Observations and Theory of Dynamical Triggers for Star Formation | |Observations and Theory of Dynamical Triggers for Star Formation | ||
| − | | | + | |The paper by The author on triggered star-formation. |
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|[http://adsabs.harvard.edu/abs/2009ApJS..181..321E Evans et al. (2009)] | |[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 | |The Spitzer c2d Legacy Results: Star-Formation Rates and Efficiencies; Evolution and Lifetimes | ||
| − | | | + | |Discussion of efficiencies, rates and lifetimes. |
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|[http://adsabs.harvard.edu/abs/1997AJ....114.1106M Megeath & Wilson (1997)] | |[http://adsabs.harvard.edu/abs/1997AJ....114.1106M Megeath & Wilson (1997)] | ||
|The NGC 281 west cluster. I. Star formation in photoevaporating clumps. | |The NGC 281 west cluster. I. Star formation in photoevaporating clumps. | ||
| − | | | + | |Establishes NGC 281 as a site of triggered SF. |
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|[http://adsabs.harvard.edu/abs/1997AJ....113.2116G Guetter & Turner (1997)] | |[http://adsabs.harvard.edu/abs/1997AJ....113.2116G Guetter & Turner (1997)] | ||
|IC 1590, A Young Cluster Embedded in the Nebulosity of NGC 281 | |IC 1590, A Young Cluster Embedded in the Nebulosity of NGC 281 | ||
| − | | | + | |The seminal paper on NGC 281. |
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|[http://adsabs.harvard.edu/abs/2009ApJS..181..321E Evans et al. (2009)] | |[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 | |The Spitzer c2d Legacy Results: Star-Formation Rates and Efficiencies; Evolution and Lifetimes | ||
| − | | | + | |How do we determine efficiencies and rates. |
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Revision as of 01:17, 10 February 2013
Abstract
A short, one or two paragraph, summary of the main points:
- Scientific goals of the proposal
- Proposed observations
Science Introduction and Context
Topics to consider when writing this section.
- Background -- The broad picture.
- Why is star-formation important? (LYNN)
- What do we know about star-formation. We will likely trim this to suit our goals as the proposal matures? (LYNN)
- What are the big unknowns? (LYNN)
| Paper | Title | Description | Comments | Assignment |
|---|---|---|---|---|
| NITARP pages | Our internal NITARP pages from Luisa, me and others. These are okay because they do comprise your source of knowledge on the subject. | |||
| McKee & Osteriker (2007) | Theory of Star Formation | Review article | Available for free via the arXiv link. | |
| Larson (2003) | The physics of star formation. |
- This work
- What aspect of star formation will we address in this work? (PEGGY)
- What is star formation rate? (PEGGY)
- How does triggered star formation work? (PEGGY)
- How is triggered star formation and star formation rates useful in understanding star formation process? (PEGGY)
| Paper | Title | Description | Comments | Assignment |
|---|---|---|---|---|
| Elmegreen (1998) | Observations and Theory of Dynamical Triggers for Star Formation | The paper by The author on triggered star-formation. | ||
| Evans et al. (2009) | The Spitzer c2d Legacy Results: Star-Formation Rates and Efficiencies; Evolution and Lifetimes | Discussion of efficiencies, rates and lifetimes. |
- This work (cont.)
- What target did we pick? (MELISSA)
- What do we know about NGC 281? (MELISSA)
- What is the evidence for triggered star formation in NGC 281? (MELISSA)
- What is the evidence for young stars in NGC 281? (MELISSA)
| Paper | Title | Description | Comments | Assignment |
|---|---|---|---|---|
| Megeath & Wilson (1997) | The NGC 281 west cluster. I. Star formation in photoevaporating clumps. | Establishes NGC 281 as a site of triggered SF. | ||
| Guetter & Turner (1997) | IC 1590, A Young Cluster Embedded in the Nebulosity of NGC 281 | The seminal paper on NGC 281. |
- This work (cont.)
- What Observations do we propose to do? (CAROL)
- What/which properties of NGC 281 do we wish to study? (CAROL)
- What diagnostics will we use? (CAROL)
- How will these diagnostics tell us about our proposed goals/question to study? (CAROL)
| Paper | Title | Description | Comments | Assignment |
|---|---|---|---|---|
| Fischer et al. (2012) | Results from HOPS: A Multiwavelength Census of Orion Protostars | Studying protostars with Herschel | ||
| Evans et al. (2009) | The Spitzer c2d Legacy Results: Star-Formation Rates and Efficiencies; Evolution and Lifetimes | How do we determine efficiencies and rates. | ||
| Dunham et al. (2008) | Identifying the Low-Luminosity Population of Embedded Protostars in the c2d Observations of Clouds and Cores | Why do we need data at Herschel wavelengths. |
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?
| Paper | Title | Description | Comments | Assignment |
|---|---|---|---|---|
- What tools will we use?
- To work with the data
- To produce the diagnostic plots.
| Paper | Title | Description | Comments | Assignment |
|---|---|---|---|---|
Educational/Outreach plan
- The education angle for the general public.
- Implication for public education?
- Press release?
- Image release?
