10 ENGLISH BOOKS RELATING TO «X-RAY BURSTER»
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Jesse Russell, Ronald Cohn, 2012
Compact Stellar X
Perioda Nature of Source (hrs) modulation X-ray type X1820–303 0.19 X-ray
Burster, globular cluster 4U 1850–087 0.34 UV Burster, globular cluster X1626–
673 0.7 opt sideband Burster, Pulsar X1832–330 0.73 UV Burster, globular
Walter Lewin, Michiel van der Klis, 2006
Discovering the Universe: From the Stars to the Planets
The source, called an X-ray burster, emits X rays at a constant low level; then,
suddenly and without warning, an abrupt increase occurs, followed by a gradual
decline. A typical burst lasts for 20 s. Several dozen X-ray bursters have been ...
Neil F. Comins, William J. Kaufmann, 2008
Binaries: Cygnus X
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Firefly Astronomy Dictionary
X-RAY BURSTER the X-ray emission. In other cases, expansion of the normal
star in the course of its evolution results in a flow of gas toward the collapsed star.
This matter forms an accretion disk of hot material which emits X-rays. SEE ALSO
Russian Space Probes: Scientific Discoveries and Future Missions
GRS 1716-249, black hole candidate; • IE 1740.7-2942, the great annihilator; •
GRS 1758-258, hitherto unknown X-ray burster, black hole candidate; • GX 1+4,
X-ray pulsar; • GX 354-0, X-ray burster; • Terzan II, X-ray burster; • SLX 1735-269,
Brian Harvey, Olga Zakutnyaya, 2011
Universe: The Solar System
An X-ray burster is a member of a binary system that accretes matter from its
companion star, then releases nuclear energy when the accreted matter
undergoes thermonuclear reactions. By contrast, a burst from a magnetar is a
release of ...
Roger Freedman, Robert Geller, William J. Kaufmann, 2010
New Cosmic Horizons: Space Astronomy from the V2 to the ...
This was the first X-ray burster discovery to be announced. (J. Grindlay et al, ApJ
205 (1976), p. L128. Reprinted with permission from The Astrophysical Journal.}
1 820-30 emitted two very brief bursts of X-rays in the 1 .3 to 7 keV range (see ...
High Resolution X
Spectroscopy of Cosmic Plasmas: IAU ...
1 shows hard energy part of the synthetic spectrum of an X-ray burster with Tg =
10+" K, assuming low gravity log g = 14.0, and iron number abundance 10 times
the solar value (DOTTED LINE). Horizontal axis gives decimal logarithm of ...
International Astronomical Union. Colloquium, Paul Gorenstein, Martin V. Zombeck, 1990
Accretion-powered Compact Binaries
... of Astrophysics, Nagoya University 'Cosmic Radiation Laboratory, The Institute
of Physical and Chemical Research ABSTRACT The Rapid Burster (MXB1730—
335) is a unique X-ray burster from which both type I and II bursts are observed.
Christopher W. Mauche, 2003