Multi-wavelength monitoring of GRS 1915+105

Details Multi-wavelength monitoring of GRS 1915+105 Multi-wavelength monitoring of GRS 1915+105

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aipc..410..892b&link_type=abstract

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

Computer Science

Gamma-Ray Sources, Gamma-Ray Bursts, Gamma-Ray, Black Holes, Infrared, Radio, Microwave, Luminosities, Magnitudes, Effective Temperatures, Colors, And Spectral Classification

Scientific paper

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.

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