Characteristics of AGB stars in the ISOAGAL, MACHO and other databases

Details Characteristics of AGB stars in the ISOAGAL, MACHO and other databases Characteristics of AGB stars in the ISOAGAL, MACHO and other databases

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003assl..283...43g&link_type=abstract

In: Mass-losing pulsating stars and their circumstellar matter. Workshop, May 13-16, 2002, Sendai, Japan, edited by Y. Nakada, M

Astronomy and Astrophysics

Astrophysics

Miras, Semi-Regular Variables, Isogal, Denis, Macho, 2Mass

Scientific paper

This contribution summarizes briefly some previous findings based on ISOGAL, MACHO and DENIS observations and goes on to include outlines of two projects now in progress: (I) A complete sample of M stars in the Baade's Window NGC 6522 field is being investigated using the MACHO, ISOGAL, DENIS and 2MASS databases to determine how variability and mass-loss are related to spectral sub-type. (II) The (MACHO) light curves of the defining stars of the infrared LMC mira period-luminosity relations are being analysed to check on their periods and to determine whether new information can reduce the scatter.

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