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Akademický článek
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Autor:
Kenneth Dalton
Publikováno v:
Journal of High Energy Physics, Gravitation and Cosmology. :651-654
A black hole model is proposed in which a neutron star is surrounded by a neutral gas of electrons and positrons. The gas is in a completely degenerate quantum state and does not radiate. The pressure and density in the gas are found to be much less
Publikováno v:
Chinese Astronomy and Astrophysics. 40:198-209
The formation of jets is closely related with the black hole mass and black hole spin, to study the correlations of jet power with the black hole mass and black hole spin is of significant importance for understanding the jet formation and structure.
Publikováno v:
Astronomische Nachrichten. 336:840-844
An appraisal of the behavior of stellar entropy along stellar evolution is made. It is shown that the entropy per baryon of a star of a fixed baryon number decreases monotonically with increasing compactness of the star. The same entropy per baryon i
Autor:
Yuri Cavecchi, Manuel Linares, M. Armas Padilla, Nathalie Degenaar, Rudy Wijnands, Arash Bahramian, Diego Altamirano, Craig O. Heinke
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 454(2), 1371-1386. Oxford University Press
We search the literature for reports on the spectral properties of neutron-star low-mass X-ray binaries when they have accretion luminosities between 1E34 and 1E36 ergs/s. We found that in this luminosity range the photon index (obtained from fitting
Autor:
Trivedi Rajesh
Publikováno v:
International Journal of Astronomy and Astrophysics. :11-14
A sufficiently large star will collapse to form a Black Hole Singularity due to Gravitational Pressure beyond Neutron Degeneracy. A Black Hole exhibits extremely strong Gravitational attraction that no particle or electromagnetic radiation can escape
Publikováno v:
Galaxies, Vol 5, Iss 1, p 15 (2017)
Galaxies; Volume 5; Issue 1; Pages: 15
Galaxies; Volume 5; Issue 1; Pages: 15
We study the structure and evolution of the hyperaccreting disks and outflows in the gamma ray bursts central engines. The torus around a stellar mass black hole is composed of free nucleons, Helium, electron-positron pairs, and is cooled by neutrino
Autor:
Jehangir Ahmad Dar
Publikováno v:
International Journal of Astronomy and Astrophysics. :414-418
The mass limit of neutron star has still remained a mystery. The existing Tolman-Oppenheimer-Volkoff (TOV) equation for calculating the limit always gives different values, by introducing different assumptions and having been predicted like 0.7 Mo, 3
Autor:
Hans-Thomas Janka
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 434:1355-1361
Integrating trajectories of low-mass X-ray binaries containing black holes within the Galactic potential, Repetto, Davies & Sigurdsson recently showed that the large distances of some systems above the Galactic plane can only be explained if black ho