Zobrazeno 1 - 10
of 1 362
pro vyhledávání: '"Eddington luminosity"'
Autor:
Saha, Prasenjit, author, Taylor, Paul A., author
Publikováno v:
The Astronomers' Magic Envelope : An Introduction to Astrophysics Emphasizing General Principles and Orders of Magnitude, 2018.
Externí odkaz:
https://doi.org/10.1093/oso/9780198816461.003.0007
Autor:
R. Yamamoto, Jun Fukue
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 502:5797-5807
We examine general relativistic radiatively-driven spherical winds, using the basic equations for relativistic radiation hydrodynamics under the moment formalism. Moment equations are often closed, using the equilibrium diffusion approximation, which
Autor:
R. A. Burenin, P. S. Medvedev, E. A. Nikolaeva, I. A. Zaznobin, Roman Krivonos, E. V. Filippova, Marat Gilfanov, R. A. Sunyaev, M. V. Eselevich, G. A. Khorunzhev, I. F. Bikmaev, A. R. Lyapin, G. S. Uskov, E. Irtuganov, S. Yu. Sazonov
Publikováno v:
Astronomy Letters. 47:71-87
We present the results of our identification of eight objects from the preliminary catalogue of X-ray sources detected in the 4–12 keV energy band by the Mikhail Pavlinsky ART-XC telescope onboard the SRG observatory during the first all-sky survey
Restrictions on the Parameters of Black Hole and Plasma in the Vicinity of the Source Sagittarius A*
Autor:
S. V. Chernov
Publikováno v:
Astronomy Reports. 65:110-125
Estimates for the parameters of accretion plasma flows and the central black hole by comparing the MHD model numerical calculations with observations for the center of our Galaxy Sagittarius A* in the radio range are obtained. The accretion flow was
Autor:
Zsolt Paragi, J. B. R. Oonk, Xiang Liu, Ilse van Bemmel, Xiaolong Yang, Jun Yang, Jun Yi Koay, Tao An, S. Komossa, C. S. Reynolds, Qingwen Wu, Feng Yuan
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 502(1), L61-L65
Broad Balmer emission lines in active galactic nuclei (AGN) may display dramatic changes in amplitude, even disappearance and re-appearance in some sources. As a nearby galaxy at a redshift of z = 0.0264, Mrk 590 suffered such a cycle of Seyfert type
Publikováno v:
Astrophysical Bulletin. 76:6-38
Ultraluminous X-ray sources (ULXs) were identified as a separate class of objects in 2000 based on data from the Chandra X-Ray Observatory. These are unique objects: their X-ray luminosities exceed the Eddington limit for a typical stellar-mass black
Autor:
J. C. A. Miller-Jones, Rob Fender, G. E. Anderson, W. Raja, Patrick Woudt, Matthew Whiting, Jai Verdhan Chauhan, B. S. Koribalski, P. F. L. Jacob, James R. Allison, Elizabeth K. Mahony, S. Corbel, F. Carotenuto, Aidan Hotan
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 501 (1), pp.L60-L64. ⟨10.1093/mnrasl/slaa195⟩
Monthly Notices of the Royal Astronomical Society, 2021, 501 (1), pp.L60-L64. ⟨10.1093/mnrasl/slaa195⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 501 (1), pp.L60-L64. ⟨10.1093/mnrasl/slaa195⟩
Monthly Notices of the Royal Astronomical Society, 2021, 501 (1), pp.L60-L64. ⟨10.1093/mnrasl/slaa195⟩
We present HI absorption spectra of the black hole candidate X-ray binary (XRB) MAXI J1348-630 using the Australian Square Kilometre Array Pathfinder (ASKAP) and MeerKAT. The ASKAP HI spectrum shows a maximum negative radial velocity (with respect to
Autor:
Mitchell C. Begelman, Eric R. Coughlin
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 499:3158-3177
Relativistic jets, or highly collimated and fast-moving outflows, are endemic to many astrophysical phenomena. The jets produced by gamma-ray bursts and tidal disruption events are accompanied by the accretion of material onto a black hole or neutron
Autor:
Barry McKernan, Nicholas P. Ross, K. E. Saavik Ford, Daniel Stern, Matthew J. Graham, Giorgio Calderone
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 498:2339-2353
We report on three redshift $z>2$ quasars with dramatic changes in their C IV emission lines, the first sample of changing-look quasars (CLQs) at high redshift. This is also the first time the changing-look behaviour has been seen in a high-ionisatio
Autor:
Marina Orio
Publikováno v:
Advances in Space Research. 66:1193-1201
High resolution X-ray spectra of classical and recurrent novae in outburst have opened a new window into the nova phenomenon, allowing to observe both the hydrogen burning white dwarf (WD) with only a very thin atmosphere on top, and violent phenomen