A non-linear mathematical model for the X-ray variability classes of the microquasar GRS 1915+105 – I. Quiescent, spiking states, and quasi-periodic oscillations
Author:
Affiliation:
1. INAF, IAPS, via del Fosso del Cavaliere 100, I-00113 Roma, Italy
2. INAF, IASF Palermo, via U. La Malfa 153, I-90146 Palermo, Italy
3. Sapienza Università di Roma, Piazzale Aldo Moro, 5, I-00185 Roma, Italy
Abstract
Funder
Agenzia Spaziale Italiana
Institut sur la Nutrition et les Aliments Fonctionnels
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/staa1124/33129511/staa1124.pdf
Reference65 articles.
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4. TURBULENT CELLS IN STARS: FLUCTUATIONS IN KINETIC ENERGY AND LUMINOSITY
5. Discovery of a 34 Hz quasi-periodic oscillation in the X-ray emission of GRS 1915+105
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1. A spectral study of GRS 1915+105 during its March 2017 NuSTAR observations;Monthly Notices of the Royal Astronomical Society;2023-12-18
2. A new variability pattern in GRS 1915+105 with NICER and Insight-HXMT observations;Monthly Notices of the Royal Astronomical Society;2023-08-09
3. Stochastic nonlinear self-oscillatory model of an accretion disk for the X-ray bursting of the microquasar GRS 1915+105;Contributions of the Astronomical Observatory Skalnaté Pleso;2023-02-01
4. Stochastic dynamical description of κ and ρ bursting classes of the microquasar GRS 1915+105;Monthly Notices of the Royal Astronomical Society;2022-10-12
5. The Slow Heartbeats of an Ultraluminous X-Ray Source in NGC 3621;The Astrophysical Journal;2020-08-05
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