The Light Variation of OH/IR Stars in the Galactic Bulge Region

Details The Light Variation of OH/IR Stars in the Galactic Bulge Region The Light Variation of OH/IR Stars in the Galactic Bulge Region

May 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aspc..439..265z&link_type=abstract

The Galactic Center: a Window to the Nuclear Environment of Disk Galaxies. Proceedings of a workshop held at Shanghai, China on

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The OH/IR stars are oxygen-rich, cool giants that lose matter in the Asymptotic Giant Branch (AGB) phase. In the Galactic Bulge region, they have a visible light variation. From the time-series photometric databases in the V-band from the MACHO, OGLE, ASAS and EROS-2 projects, we retrieved the light curve of 29 OH(1612MHz)/IR in the bulge. By the PDM method, the characteristics of their light variation are analyzed.

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