Multi-wavelength monitoring of GRS 1915+105

Bibcode
1997AIPC..410..892B
DOI
10.1063/1.54159
Bandyopadhyay, R.; Martini, P.; Gerard, E.; Charles, P. A.; Wagner, R. M.; Shrader, C.; Shahbaz, T.; Mirabel, I. F.
Bibliographical reference

The fourth compton symposium. AIP Conference Proceedings, Volume 410, pp. 892-896 (1997).

Advertised on:
5
1997
Number of authors
8
IAC number of authors
0
Citations
0
Refereed citations
0
Description
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 All Sky Monitor and BATSE, two-frequency data from the Nancay radio telescope, and infrared photometry from the 1.8m Perkins telescope at Lowell 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.
Type
Non-refereed
Gamma-ray sources
Gamma-ray bursts
Black holes

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