Results 11 to 20 of about 8,164 (262)
Supercollapsars and their X-ray bursts [PDF]
Monthly Notices of the Royal Astronomical Society: Letters, 2010 Abstract The very first stars in the Universe can be very massive, up to 103 M⊙. If born in large numbers, such massive stars can have a strong impact on the subsequent star formation, producing strong ionizing radiation and contaminating the primordial gas with heavy elements.
Komissarov, S. S., Barkov, M. V.
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X-Ray Bursts of Nuclear Origin [PDF]
Highlights of Astronomy, 1977 The fate of nuclear energy carried by matter accreted onto a neutron star was considered e.g. by Rosenbluth et al. (1973). They examined pycnonuclear reactions on an originally cold star, and found that the whole star is thereby heated up to 106−107 °K. The thermonuclear reactions that can be ignited then, have been studied by Hansen and Van Horn (1975)
L. Maraschi, A. Cavaliere
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Detection of X-Ray Bursts in Astronomical Time Series: The Burst of GRO J1744-28 as an Example
The Astrophysical Journal, 2023 To automatically, accurately, and quickly detect local changes in time-series data continuously emitted by X-ray sources, an autoencoder-based unsupervised learning anomaly detection method is proposed.
Hongyang Zhao +4 more
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The Astrophysical Journal, 2023 The Space-based multiband astronomical Variableonboard computing resources. This Object Monitor (SVOM) is a Sino–French space mission targeting high-energy transient astrophysical objects such as gamma-ray bursts.
Shaymaa Hussein +5 more
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Accretion rates in X-ray bursting sources [PDF]
The Astrophysical Journal, 1994 21 pages ...
LAPIDUS I. +2 more
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Solar Physics, 1985 The major results from SMM are presented as they relate to our understanding of the energy release and particle transportation processes that lead to the high-energy X-ray aspects of solar flares. Evidence is reviewed for a 152–158 day periodicity in various aspects of solar activity including the rate of occurrence of hard X-ray and gamma-ray flares ...
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Reanalysis of the X-Ray-burst-associated FRB 200428 with Insight-HXMT Observations
The Astrophysical Journal, 2023 A double-peak X-ray burst from the Galactic magnetar SGR J1935+2154 was discovered to be associated with the two radio pulses of FRB 200428 separated by 28.97 ± 0.02 ms.
M. Y. Ge +17 more
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X-Ray Bursting Neutron Stars [PDF]
Symposium - International Astronomical Union, 1987 The maximum peak luminosity of the X-ray bursts from a burster is most likely interpreted as the Eddington luminosity of a helium-rich envelope surrounding a neutron star. If this interpretation is true, we can obtain a relation between the mass and the radius of the neutron star in terms of the maximum effective temperature of bursts.
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Геодинамика и тектонофизика, 2019 Seven gamma-ray bursts – GRB 130907A, GRB 140311B, GRB 140129B, GRB 160227A, GRB 120404A, GRB 110801A, and GRB 120811C were observed by the MSU MASTER (Mobile Astronomical System of TElescope Robots) Global Network.
V. M. Lipunov +31 more
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The Game of Life on a Magnetar Crust: From Gamma-Ray Flares to FRBs
The Astrophysical Journal Letters, 2023 This Letter presents a model to unify the diverse range of magnetar activity, through the building and release of elastic stress from the crust. A cellular automaton drives both local and global yielding of the crust, leading to braiding of coronal loops
S. K. Lander
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