4.6 Article

86 GHz SiO maser survey of late-type stars in the inner Galaxy - II. Infrared photometry of the SiO target stars

Journal

ASTRONOMY & ASTROPHYSICS
Volume 418, Issue 1, Pages 103-116

Publisher

E D P SCIENCES
DOI: 10.1051/0004-6361:20034488

Keywords

stars : AGB and post-AGB; infrared : stars; stars : variables : general; stars : circumstellar matter; masers; Galaxy : stellar content

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We present a compilation and study of DENIS, 2MASS, ISOGAL, MSX and IRAS 1-25 mum photometry for a sample of 441 late-type stars in the inner Galaxy, which we previously searched for 86 GHz SiO maser emission (Messineo et al. 2002). The comparison of the DENIS and 2MASS J and K-S magnitudes shows that most of the SiO targets are indeed variable stars. The MSX colours and the IRAS [12]-[25] colour of our SiO targets are consistent with those of Mira type stars with dust silicate feature at 9.7 mum feature in emission, indicating only a moderate mass-loss rate.

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