The evolution from visible to infrared variable AGB stars: What can DENIS contribute to this study?

Details The evolution from visible to infrared variable AGB stars: What can DENIS contribute to this study? The evolution from visible to infrared variable AGB stars: What can DENIS contribute to this study?

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.217..143b&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 217, no. 1-2, p. 143-144

Astronomy and Astrophysics

Astronomy

Asymptotic Giant Branch Stars, Infrared Astronomy, Infrared Stars, Sky Surveys (Astronomy), Stellar Evolution, Stellar Mass, Stellar Mass Ejection, Stellar Models, Variable Stars, Astronomical Photometry, Detection, Infrared Astronomy Satellite, Near Infrared Radiation, Stellar Magnitude, Visibility

Scientific paper

Results of the Vassiliadis and Wood (1993) model for the evolution on
the Asymptotic Giant Branch (AGB) are used to study how Deep
Near-Infrared Survey (DENIS) can complement an optical and Infrared
Astronomy Satellite (IRAS) based study of Long Period Variable (LPV) AGB
stars in a field towards the galactic bulge.

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