Carbon stars in infrared surveys

Details Carbon stars in infrared surveys Carbon stars in infrared surveys

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.217..141g&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 217, no. 1-2, p. 141-142

Astronomy and Astrophysics

Astronomy

Asymptotic Giant Branch Stars, Carbon Stars, Galactic Structure, Infrared Astronomy, Near Infrared Radiation, Sky Surveys (Astronomy), Spatial Distribution, Classifications, Cross Correlation, Detection, Diagrams, Infrared Astronomy Satellite, Milky Way Galaxy, Predictions, Stellar Color, Stellar Models

Scientific paper

In order to prepare the analysis of the forthcoming near-IR surveys (Deep Near-Infrared Survey (DENIS) and Two Micron All Sky Survey (2MASS)) and to interpret them in terms of galactic structure and Asymptotic Giant Branch (AGB) evolution, we present model predictions of AGB distributions in K, in 12 micrometer and in (J-K, 12-25) space, as they will be obtained from these surveys, cross-correlated with Infrared Astronomy Satellite (IRAS) Catalog. The simulations have been made by adding the AGB to the Besancon model.

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