Answers are grounded in this paper and cite their sources.
We report the observation of events with fast (≤1 hr) time variability in Very Large Array observations of the Galactic superluminal source GRS 1915+105. The database consists of observations made at 67 epochs over 3 yr. We have detected fast variations on three occasions. Here we report the most remarkable of the events, observed in 1995 September 6. Over a period of approximately 2 hr, the 3.6 cm flux density of GRS 1915+105 showed several clear sinusoidal oscillations with period of 30.2 ± 0.4 minutes, going from ~40 to ~65 mJy. We discuss possible scenarios for the production of this fast sinusoidal variation in the radio flux density and propose that the variability could be the result of a hot spot orbiting the collapsed companion of the binary system.
No takes yet. Share an insight, caveat, or question.
Rodrı́guez et al. (1997) studied this question.
Synapse has enriched 10 related papers. Consider them for comparative context: