A Time-dependent Leptonic Model for Microquasar Jets: Application to LS I +61 303
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
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1. Discovering the Mass-Scaled Damping Timescale from Microquasars to Blazars;The Astrophysical Journal Letters;2024-05-01
2. Optical microflares in LS I +61 303 and the search for their multiwavelength counterpart;Astronomy & Astrophysics;2022-06
3. THE MULTI-WAVELENGTH CHARACTERISTICS OF THE TeV BINARY LS I+61°303;The Astrophysical Journal;2016-05-31
4. POSSIBLE CHANGES OF STATE AND RELEVANT TIMESCALES FOR A NEUTRON STAR IN LS I +61°303;The Astrophysical Journal;2012-08-27
5. DETECTION OF THE γ-RAY BINARY LS I +61°303 IN A LOW-FLUX STATE AT VERY HIGH ENERGY γ-RAYS WITH THE MAGIC TELESCOPES IN 2009;The Astrophysical Journal;2012-01-25
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