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Title:
The Orbital Period of 4U 1210-64
Authors:
Corbet, R. H. D.; Mukai, K.
Publication:
The Astronomer's Telegram, #1861
Publication Date:
12/2008
Origin:
ATEL
Keywords:
X-ray, Binaries, Cataclysmic Variables, Neutron Stars
Bibliographic Code:
2008ATel.1861....1C

Abstract

The nature of 4U 1210-64 (= 1ES 1210-646) is not yet clear. Revnivtsev et al. (2007, ATEL #1253) propose that 4U 1210-64 may be an intermediate polar while Masetti et al. (2008, A&A in press, arXiv:0811.4085v1) find that the source is a high-mass X-ray binary. The RXTE ASM light curve of 4U 1210-64 obtained between MJD 50,087 and 54,797 shows that the source has exhibited different states with relatively low or high flux.
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