Ammonia on YSOs IRAS sources (Molinari+ 1996)

Details Ammonia on YSOs IRAS sources (Molinari+ 1996) Ammonia on YSOs IRAS sources (Molinari+ 1996)

Apr 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ycat..33080573m&link_type=abstract

VizieR On-line Data Catalog: J/A+A/308/573. Originally published in: 1996A&A...308..573M

Computer Science

Ysos, Radio Lines

Scientific paper

We present observations of NH3 (1,1) and (2,2) lines flux-limited samples of IRAS sources selected according to colour criteria which should result in a high fraction of Young Stellar Objects. The first sample contains sources (named 'LOW') whose evolutionary status is essentially unknown, while the second sample contains sources (named 'HIGH') possibly associated with ultracompact HII regions, the distinction being based on the IRAS [25-12] colour. (2 data files).

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