Large-amplitude variables near the Galactic Centre

Details Large-amplitude variables near the Galactic Centre Large-amplitude variables near the Galactic Centre

Feb 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001mnras.321...77g&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 321, Issue 1, pp. 77-95.

Other

39

Surveys, Stars: Agb And Post-Agb, Stars: Variables: Other, Galaxy: Centre

Scientific paper

We report here the results of a 4-yr K-band (2.2μm) survey for large-amplitude variable stars in a 24×24arcmin2 area centred on the Galactic Centre. A total of 409 likely long-period variables (LPVs) were detected, for which positions, amplitudes, average magnitudes and periods were obtained whenever possible. The surface density of LPVs is more than ten times greater than in the Sgr I Baade window at l=-1.37°, b=-2.63°. The limits of completeness arising from interstellar and circumstellar absorption are discussed. Most of the area suffers interstellar extinction of 2040mag), which affects the probability of detecting variables, occurs in less than 25per cent of the area. Almost all of the LPVs are Miras or OH/IR stars, with periods ranging from 150d to about 800d. K-band counterparts have been found for 59per cent of the 109 known OH sources in the field. The average period of the variables found is 427d, while that of the OH/IR stars is 524d. For comparison, the average period in the Sgr I window, which contains no known OH/IR stars, is 333d and only two stars are detected with P>600d. The survey field also contains a number of long-period, large-amplitude variables that are not OH emitters.

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