GRS 1915+105 or V1487 Aquilae is an
X-ray binary star system which features a regular star and a
black hole
A black hole is a region of spacetime where gravitation, gravity is so strong that nothing, including light or other Electromagnetic radiation, electromagnetic waves, has enough energy to escape it. The theory of general relativity predicts t ...
. It was discovered on August 15, 1992 by the WATCH all-sky monitor aboard
Granat.
[ "GRS" stands for "GRANAT source", "1915" is the ]right ascension
Right ascension (abbreviated RA; symbol ) is the angular distance of a particular point measured eastward along the celestial equator from the Sun at the March equinox to the (hour circle of the) point in question above the earth.
When paired w ...
(19 hours and 15 minutes) and "105" reflects the approximate declination
In astronomy, declination (abbreviated dec; symbol ''δ'') is one of the two angles that locate a point on the celestial sphere in the equatorial coordinate system, the other being hour angle. Declination's angle is measured north or south of the ...
(10 degrees and 56 arcminutes). The near-infrared counterpart was confirmed by spectroscopic observations.[ The binary system lies 11,000 parsecs away][ in ]Aquila
Aquila may refer to:
Arts, entertainment, and media
* ''Aquila'', a series of books by S.P. Somtow
* ''Aquila'', a 1997 book by Andrew Norriss
* ''Aquila'' (children's magazine), a UK-based children's magazine
* ''Aquila'' (journal), an or ...
. GRS 1915+105 is the heaviest of the stellar black holes so far known in the Milky Way Galaxy,[ with 10 to 18 times the ]mass of the Sun
The solar mass () is a standard unit of mass in astronomy, equal to approximately . It is often used to indicate the masses of other stars, as well as stellar clusters, nebulae, galaxies and black holes. It is approximately equal to the mass ...
.[ It is also a microquasar, and it appears that the black hole rotates at least 950 times per second, close to the maximum of 1,150 times per second, with a spin parameter value between 0.82 and 1.00 (maximum possible value).][
]
Galactic superluminal source
In 1994, GRS 1915+105 became the first known galactic source that ejects material with apparent superluminal motion
In astronomy, superluminal motion is the apparently faster-than-light motion seen in some
radio galaxies, BL Lac objects, quasars, blazars and recently also in some galactic sources called microquasars. Bursts of energy moving out along the rel ...
velocities.[
Observations with high resolution radio telescopes such as ]VLA VLA or vla may refer to:
Organizations
* Vermont Library Association, professional organization for librarians from Vermont
* Veterinary Laboratories Agency, a UK government agency for researching animal and public health
* Victoria Legal Aid, an ...
, MERLIN
Merlin ( cy, Myrddin, kw, Marzhin, br, Merzhin) is a mythical figure prominently featured in the legend of King Arthur and best known as a mage, with several other main roles. His usual depiction, based on an amalgamation of historic and le ...
, and VLBI show a bi-polar outflow of charged particles, which emit synchrotron radiation
Synchrotron radiation (also known as magnetobremsstrahlung radiation) is the electromagnetic radiation emitted when relativistic charged particles are subject to an acceleration perpendicular to their velocity (). It is produced artificially in ...
at radio frequencies. These studies have shown that the apparent superluminal motion is due to a relativistic effect known as relativistic aberration, where the intrinsic velocity of ejecta is actually about 90% the speed of light.[
]
Growth regulation
Repeat observations by the Chandra X-Ray Observatory over the period of a decade have revealed what may be a mechanism for self-regulation of the rate of growth of GRS 1915+105. The jet of materials being ejected is occasionally choked off by a hot wind blowing off the accretion disk. The wind deprives the jet of materials needed to sustain it. When the wind dies down, the jet returns.[
]
See also
* GRO J1655-40
GRO J1655-40 is a binary star consisting of an evolved F-type primary star and a massive, unseen companion, which orbit each other once every 2.6 days in the constellation of Scorpius.
Gas from the surface of the visible star is accr ...
References
External links
A Very Massive Stellar Black Hole in the Milky Way Galaxy
November 28, 2001 (ESO)
Image V1487 Aquilae
O maior buraco negro estelar da Via Láctea (The biggest stellar black hole of the Milky Way)
- in Portuguese.
The micro quasar GRS 1915+105
INTEGRAL Science Data Centre
{{DEFAULTSORT:GRS 1915+105
X-ray binaries
Aquila (constellation)
Microquasars
Aquilae, V1487
K-type giants