On the optical extinction and distance of GRS 1915+105
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361:20034028/pdf
Reference48 articles.
1. CO-to-H2Conversion Factor in Galaxies
2. An Unstable Central Disk in the Superluminal Black Hole X-Ray Binary GRS 1915+105
3. A Unified Model for the Spectral Variability in GRS 1915+105
4. Diffuse Gamma-Ray Emission in the Galactic Plane from Cosmic-Ray, Matter, and Photon Interactions
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1. Fast infrared winds during the radio-loud and X-ray obscured stages of the black hole transient GRS 1915+105;Astronomy & Astrophysics;2023-12
2. The Black Hole Candidate Swift J1728.9–3613 and the Supernova Remnant G351.9–0.9;The Astrophysical Journal;2023-04-01
3. Origins of the Long-term Variability of the Near-infrared Emission of the Black Hole X-Ray Binary GRS 1915+105 in the X-Ray Low Luminous State;The Astrophysical Journal;2021-08-01
4. The Black Hole Spin in GRS 1915+105, Revisited;The Astrophysical Journal;2021-06-01
5. The obscured X-ray binaries V404 Cyg, Cyg X–3, V4641 Sgr, and GRS 1915+105;Astronomy & Astrophysics;2020-07
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