Multi-wavelength monitoring of GRS1915+105

被引：0

作者：

Bandyopadhyay, R ^{[1
]}

Martini, P ^{[1
]}

Gerard, E ^{[1
]}

Charles, PA ^{[1
]}

Wagner, RM ^{[1
]}

Shrader, C ^{[1
]}

Shahbaz, T ^{[1
]}

Mirabel, IF ^{[1
]}

机构：

[1] Univ Oxford, Oxford OX1 2JD, England

来源：

PROCEEDINGS OF THE FOURTH COMPTON SYMPOSIUM, PTS 1 AND 2: PT 1: THE COMPTON OBSERVATORY IN REVIEW; PT 2: PAPERS AND PRESENTATIONS | 1997年 / 410期

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Since its discovery in 1992, the superluminal X-ray transient GRS 1915+105 has been extensively observed in an attempt to understand its behaviour, We present here preliminary results from a multi-wavelength campaign undertaken from July to September 1996. This study includes X-ray data from the RXTE AII Sky Monitor and BATSE, two-frequency data from the Nancay radio telescope, and infrared photometry from the 1.8m Perkins telescope at Lower Observatory. The K-band data presented herein provide the first long-term well-sampled IR light curve of GRS 1915+105. We compare the various light curves, searching for correlations in the behaviour of the source at differing wavelengths and for possible periodicities.

引用

页码：892 / 896

页数：5