Obscured AGB in Magellanic Clouds. I. (Loup+ 1997)

Details Obscured AGB in Magellanic Clouds. I. (Loup+ 1997) Obscured AGB in Magellanic Clouds. I. (Loup+ 1997)

Feb 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997ycat..41250419l&link_type=abstract

VizieR On-line Data Catalog: J/A+AS/125/419. Originally published in: 1997A&AS..125..419L

Physics

Stars: Supergiant, Planetary Nebulae, Infrared Sources

Scientific paper

We have selected 198 IRAS sources in the Large Magellanic Cloud, and 11 in the Small Magellanic Cloud, which are the best candidates to be mass-loosing AGB stars (or possibly post-AGB stars). We used the catalogues of Schwering & Israel (1990, Cat. ) and Reid et al. (1990, Cat. ). They are based on the IRAS pointed observations and have lower detection limits than the Point Source Catalogue. We also made cross-identifications between IRAS sources and optical catalogues. (8 data files).

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