Spectral, polarization and time-lag properties of GRS 1915+105 radio oscillations

被引:32
作者
Fender, RP
Rayner, D
Trushkin, SA
O'Brien, K
Sault, RJ
Pooley, GG
Norris, RP
机构
[1] Univ Amsterdam, Astron Inst Anton Pannekoek, NL-1098 SJ Amsterdam, Netherlands
[2] Ctr High Energy Astrophys, NL-1098 SJ Amsterdam, Netherlands
[3] CSIRO, Australia Telescope Natl Facil, Epping, NSW 2121, Australia
[4] RAS, Special Astrophys Observ, Nizhnii Arkhyz 369167, Karachaevo Cher, Russia
[5] Univ Cambridge, Cavendish Lab, Mullard Radio Astron Observ, Cambridge CB3 0HE, England
关键词
binaries : close; stars : individual : GRS 1915+105; ISM : jets and outflows; infrared : stars; radio continuum : stars;
D O I
10.1046/j.1365-8711.2002.05072.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report high-sensitivity dual-frequency observations of radio oscillations from GRS 1915+ 105 following the decay of a major flare event in 2000 July. The oscillations are clearly observed at both frequencies, and the time-resolved spectral index traces the events between optically thin and thick states. While previously anticipated from sparse observations and simple theory, this is the first time a quasi-periodic signal has been seen in the radio spectrum, and is a clear demonstration that flat radio spectra can arise from the combination of emission from optically thick and thin regions. In addition, we measure the linear polarization of the oscillations, at both frequencies. at a level of about 1-2 per cent, with a flat spectrum. Cross-correlating the two light curves we find a mean delay, in the sense that the emission at 8640 MHz leads that at 4800 MHz, of around 600 s. Comparison with frequency-dependent time-delays reported in the literature reveals that this delay is variable between epochs. We briefly discuss possible origins for a varying time-delay, and suggest possible consequences.
引用
收藏
页码:212 / 218
页数:7
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