Infrared observations and energetic outburst of GRS 1915+105

Multiple near-infrared wavelengths observations, carried out since 1993 on the galactic superluminal source of relativistic ejections GRS 1915 + 105, have yielded three important results. 1) The infrared counterpart of GRS 1915 + 105 exhibits various variations in the 1.2 μm-2.2 μm band: the strongest are of ∼ 1 magnitude in a few hours and of ∼ 2 magnitudes over longer intervals of time (Chaty et al. 1996). 2) The infrared properties of GRS 1915 + 105 are strikingly similar to those of SS 433, and unlike those of any other known stellar source in the Galaxy. The absolute magnitudes, colors, and time variabilities of these two sources of relativistic ejections suggest that GRS 1915 + 105, like SS 433, consists of a collapsed object (neutron star or black hole) with a thick accretion disk in a high-mass-luminous binary system (Chaty et al. 1996). 3) During an intense and long-term X-ray outburst of GRS 1915 + 105 in 1995 August, where a pair of radio-emitting clouds emerged from the compact core in opposite directions at relativistic speeds, we observed the time-delayed reverberation of this radio flare/ejection event in the infrared wavelengths. The observed spectrum of the enhanced infrared emission suggests the appearance of a warm dust component (Mirabel et al. 1996a).