期刊
ASTRONOMY & ASTROPHYSICS
卷 380, 期 2, 页码 516-519出版社
EDP SCIENCES S A
DOI: 10.1051/0004-6361:20011390
关键词
stars : neutron; stars : individual : LSI+61 degrees 303; binaries : radio; stars : emission line, Be; X-rays : stars
An analysis of RXTE/ASM observations of the unusual binary system LSI +61 degrees 303 is presented. The X-ray light curve gives a binary period of 26.42 +/- 0.05 days, and an eccentricity of 0.30 +/- 0.04 (1 sigma). The eccentricity is determined by fitting an inverse Compton model to the X-ray light curve. These are the best determinations to date, as the optical period and eccentricity have larger uncertainties and published values of the radio period are variable. The radio outburst peak is not phase locked to the binary period, so the radio period is not the same as the binary period.
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