Warm gas towards young stellar objects in Corona Australis - Herschel/PACS observations from the DIGIT key programme

Johan E. Lindberg; Jes K. Jørgensen; Joel D. Green; Gregory J. Herczeg; Odysseas Dionatos; Neal J. Evans; Agata Karska; Susanne F. Wampfler

doi:10.1051/0004-6361/201322184

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Volume 565 (May 2014)

A&A, 565 (2014) A29

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Table 1

Observational parameters.

Region	RA	Dec	PA^a	Observing IDs	Date of observation
	(J2000.0)	(J2000.0)	[°]

IRS7A	19:01:55.3	−36:57:17.0	− 0.22	1342206990, 1342206989	2010-10-23
IRS7B	19:01:56.4	−36:57:28.3	2.47	1342207807, 1342207808	2010-11-02
IRS5A	19:01:48.1	−36:57:22.7	2.40	1342207806, 1342207805	2010-11-01

Notes. Positions give the centre coordinates of the central spaxel. All footprints are 5 × 5 spaxel grids with approximately 9.̋25 separation between the spaxel centres.

^(a)

Position angle with respect to an equatorial grid coordinate system.

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