Optical spectroscopy of GX 339-4 - I. Orbital modulation

被引:18
|
作者
Buxton, M
Vennes, S
机构
[1] Mt Stromlo & Siding Spring Observ, Res Sch Astron & Astrophys, Weston, ACT 2611, Australia
[2] Australian Natl Univ, Dept Math, Acton, ACT 0200, Australia
关键词
accretion; accretion discs; black hole physics; binaries : spectroscopic; stars : individual : GX 339-4; X-rays : binaries;
D O I
10.1046/j.1365-8711.2003.06516.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Optical spectroscopic observations of GX 339-4 were carried out between 1998 May (X-ray high state) and 1999 May (X-ray low state) over seven epochs. The equivalent width of Halpha increased during the high state and then decreased during the low state. The equivalent width of He II lambda4686 decreased over both states. The full-width at half-maximum of Halpha, Hbeta, He II lambda4686 and the Bowen blend increased from 1998 to 1999, indicating that the emission-line regions moved closer to the compact object. Hbeta shows a redshifted absorption feature at),4880 at all epochs. This line remains unidentified. Analysis of individual spectra from 1998 May 28-31 shows modulation of the radial velocities, equivalent width and VIR ratios of Halpha on the 14.86-h orbital period. The equivalent width of He II lambda4686 also varies on the orbital period. The semi-amplitude of the Ha radial velocities is K-1 = 14 km s(-1). Hence the mass function = 2 x 10(-4) M-..
引用
收藏
页码:105 / 118
页数:14
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