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| | Subject to change! Includes agenda for Summer visit. | | Subject to change! Includes agenda for Summer visit. |
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| − | =Previously Known Objects in Puppis region (Reipurth and Pettersson 1993)= | + | =Previously Known Objects in Puppis region (Reipurth and Pettersson 1993)...''fixed CG-Halpha4''= |
| | {| border="1" | | {| border="1" |
| | |Star | | |Star |
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| | |CG-Halpha 4 | | |CG-Halpha 4 |
| | |07 31 21.92 | | |07 31 21.92 |
| − | | -46 59 45.14 | + | | -46 '''''57''''' 45.14 ** |
| | |14.59 | | |14.59 |
| | |1.40 | | |1.40 |
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| | =[[CG4 Fall Work]]= | | =[[CG4 Fall Work]]= |
| − | First draft of Science Abstract:
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| − | ''We used archival Spitzer data to look for new young stellar objects (YSOs) in Cometary Globule 4 (CG4) in Puppis. CG4 is approximately 1300 parsecs and one of about 30 cometary globules in the Gum Nebula, many of which are known to be forming stars. These globules are pointed generally radially outward from the center of the Vela OB2 association, which is also forming stars. CG4 is dramatic in appearance, and that has brought it to the attention of both scientists and the public. Our team used archival Spitzer InfraRed Array Camera (IRAC) and Multiband Imaging Photometer for Spitzer (MIPS) data and 2 Micron All Sky Survey (2MASS) data, as well as optical data obtained by collaborators. We used infrared excess to find nine previously known YSOs and additional new YSOs in this region. We will primarily use infrared excess to find new YSOs. We used available data to attempt to determine legitimate cluster members, and to separate CG4’s YSOs from other objects with similar spectral energy distributions (SEDs). This research was made possible through the NASA/IPAC Teacher Archive Research Project (NITARP) and was funded by the Spitzer Science Center (SSC).'' | + | =[[CG4 Abstracts]]= |
| | + | ''Now pulled off to their own page.'' |
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| − | Please edit as you see fit.
| + | =[[CG4 Winter Mini-Workshop]]= |
| | + | NEW! See email... |
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| − | Luisa's edits:
| + | =[[CG4 AAS 2011 Meeting]]= |
| − | ''We used archival Spitzer infrared data to look for new young stellar objects (YSOs) in Cometary Globule 4 (CG4) in Puppis. CG4 is approximately 1300 parsecs away and one of about 30 cometary globules in the Gum Nebula, many of which are known to be forming stars. CG4 is dramatic in appearance, and that has brought it to the attention of both scientists and the public. Our team used archival Spitzer InfraRed Array Camera (IRAC) and Multiband Imaging Photometer for Spitzer (MIPS) data, combined with 2 Micron All Sky Survey (2MASS) data as well as optical data obtained by collaborators. We used infrared excess to investigate the properties of previously known YSOs in this region and identify additional new candidate YSOs in this region. This research was made possible through the NASA/IPAC Teacher Archive Research Project (NITARP) and was funded by the Spitzer Science Center (SSC).''
| + | ''Pictures and more'' |
| − | rationale for my changes: occasional missing words/wordsmithing. the stuff about radially pointing is indeed true, but not strictly relevant to the abstract (tho' it's appropriate for the main body of the poster in the introduction). 'we will use' = lingering sentence left over i think from editing, since it is redundant with prior sentence. stuff about separating YSOs from contaminants absolutely true, but is implicit in the statement that we've identified YSO candidates -- of course we've attempted to weed out contaminants. there should be some text on that in the main body of the poster, though, for sure.
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| − | Also, send Chelen the names of all additional authors to be listed. For example, I will write the Breck team as ...
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| − | Chelen Johnson, Rachel Crump, Anna Laorr, Kayla Mork, Emma Steinbergs, Sara Trautz, Elizabeth Wigley, Sally Caruso, Heather Balenger, Nina Killingstad, Taylor McCanna.
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| − | We will identify schools with superscripts and a key. (See previous NITARP posters [http://coolwiki.ipac.caltech.edu/index.php/Posters_and_Handouts_from_AAS_meetings] for an example.)
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| − | | |
| − | --chj
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| − | 21-September-2010
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| − | | |
| − | you should add me, of course, but also Serena Kim (Univ. Arizona). --[[User:Rebull|Rebull]] 09:09, 22 September 2010 (PDT)
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| − | | |
| − | Here's the author list ...
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| − | Chelen Johnson, Rachel Crump, Anna Laorr, Kayla Mork, Emma Steinbergs, Sara Trautz, Elizabeth Wigley, Sally Caruso, Heather Balenger, Nina Killingstad, Taylor McCanna (Breck School, Minneapolis, MN)
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| − | Luisa Rebull (SSC/IPAC/CalTech, Pasadena, CA)
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| − | Vivian Hoette (University of Chicago, Yerkes Observatory, Williams Bay, WI)
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| − | Carolyn Mallory, Michael Feig, Niyaz Mahmud, Tiffany Selic (Pierce College, Woodland Hills, CA)
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| − | Kevin McCarron (Oak Park River Forest High School, Oak Park, IL)
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| − | Constance Gartner, Jennifer VanDerMolen, Lissa Matche, Anna McCartney (Wisconsin School for the Deaf, Delavan, WI)
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| − | Lee Gamble, Mark Doering (Wisconsin Center for the Blind and Visually Impaired, Janesville, WI)
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| − | Russ Laher (SSC/IPAC/CalTech, Pasadena, CA)
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| − | Mark Legassie (SSC/IPAC/CalTech/Raytheon, Pasadena, CA)
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| − | Serena Kim (U of Arizona, Tucson, AZ)
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| − | | |
| − | --[[User:CJohnson|CJohnson]] 17:56, 22 September 2010 (CDT)
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This page will be used to assemble the pieces for the proposal we are writing.
A consolidation of all sorts of useful links, mostly culled from Luisa's email.
Previous Teams' pages
Lynds Clouds Current Research Activities and IC 2118 Current Research Activities
This page will be used to collect information during our work in Spring.
This page will be used to collect logistics information about our IPAC visit. The visit is June 14-16. (NB: HOU conference at Yerkes June 20-24.)
Subject to change! Includes agenda for Summer visit.
Previously Known Objects in Puppis region (Reipurth and Pettersson 1993)...fixed CG-Halpha4
| Star
|
RA (J2000)
|
Dec (J2000)
|
V
|
(B-V)
|
(U-B)
|
Region
|
| CG-Halpha 1
|
07 30 37.77
|
-47 25 07.21
|
>17
|
none
|
none
|
Sa 101
|
| CG-Halpha 2
|
07 30 57.63
|
-46 56 12.50
|
>17
|
none
|
none
|
Sa 101
|
| CG-Halpha 3
|
07 31 10.89
|
-47 00 33.40
|
14.99
|
1.60
|
0.91
|
Sa 101
|
| CG-Halpha 4
|
07 31 21.92
|
-46 57 45.14 **
|
14.59
|
1.40
|
0.92
|
Sa 101
|
| CG-Halpha 5
|
07 31 36.65
|
-47 00 14.13
|
15.25
|
1.26
|
0.23
|
Sa 101
|
| CG-Halpha 6
|
07 31 37.45
|
-47 00 22.19
|
14.21
|
1.42
|
0.90
|
Sa 101
|
| CG-Halpha 7
|
07 33 26.92
|
-46 48 43.51
|
13.97
|
1.19
|
0.84
|
CG 4
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| CG-Halpha 8
|
07 15 49.86
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-48 31 27.16
|
15.33
|
1.39
|
0.13
|
CG 13
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| PHalpha 92
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08 28 40.73
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-33 46 23.17
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13.38
|
1.27
|
0.91
|
CG 22
|
Sample analysis thread using Lynds 1688 (developed in the context of the Lynds Cloud team).
An adaptation of "Working with L1688" above, with specific application to our project.
Now pulled off to their own page.
NEW! See email...
Pictures and more
