Computer Science
Scientific paper
Oct 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ycat..21940043p&link_type=abstract
VizieR On-line Data Catalog: J/ApJS/194/43. Originally published in: 2011ApJS..194...43P
Computer Science
Ysos, X-Ray Sources, Photometry: Infrared, Surveys, Interstellar Medium, Interferometry, Proper Motions
Scientific paper
Corona Australis was observed with the Spitzer Infrared Array Camera (IRAC) at 3.6, 4.5, 5.8, and 8.0um and the Multiband Imaging Photometer for Spitzer (MIPS) at 24, 70, and 160um as part of two guaranteed time observation (GTO) programs (PID 6 (2004 Apr 20), 30784 (2006 Sep 25; 2007 May 29-30); PI: Fazio) as well as the Gould Belt Legacy Survey (PID 30574 (2008 May 10 & Oct 23); PI: Allen).
The regions around the previously identified YSOs IRS 5, IRS 7, and IRAS 32 (IRAS 18595-3712) were observed with the SMA (Submillimeter Array) in the dust continuum near 225GHz (~1.3mm). Observations of the IRS 7 region were made on 2006 August 20 (program 2006-03-S046), while IRAS 32 and IRS 5 were observed on 2008 June 10 and 14 (program 2008A-S074).
As a complement to the Spitzer and SMA data, we make use of multi-epoch H2 (2.12um) maps to detect jets and outflows in the CrA star-forming region to study their proper motions and identify the exciting sources.
(8 data files).
Allen Laura E.
Bourke Tyler L.
Caratti Garatti Alessio o.
Chapman Nicholas L.
Cieza Lucas. A.
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