SiO maser sources near the Galactic center

Details SiO maser sources near the Galactic center SiO maser sources near the Galactic center

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003assl..283..347d&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

Masers, Galactic Center, Agb Stars

Scientific paper

I summarize results of the SiO maser surveys of the Galactic center region, which have been made in the past 3 years at Nobeyama. About 600 color selected IRAS Sources in the inner (<3°) and outer (<10°) bulge, the 300 large amplitude variables in the nuclear disk (<12'), and the stars in the Galactic-center star cluster (<1'), have been observed with Nobeyama 45-m telescope. Expecially in the Galactic center, mapping and monitoring observations have been made. The kinematic of stars very near to the Galactic center (within a few pc) and a flare of SiO masers of IRS 10 are discussed. The flare of IRS 10 seems to repeat in every two years.

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