astro.wikisort.org - Galaxy

NGC 3115 (also called the Spindle Galaxy or Caldwell 53) is a field lenticular (S0) galaxy in the constellation Sextans. The galaxy was discovered by William Herschel on February 22, 1787.[4][5] At about 32 million light-years away from Earth, it is several times bigger than the Milky Way. It is a lenticular (S0) galaxy because it contains a disk and a central bulge of stars, but without a detectable spiral pattern. NGC 3115 is seen almost exactly edge-on, but was nevertheless mis-classified as elliptical. There is some speculation that NGC 3115, in its youth, was a quasar.

NGC 3115
Composite image of NGC 3115 from the Chandra X-ray Observatory and the Very Large Telescope
Observation data (J2000 epoch)
Constellation	Sextans
Right ascension	10h 05m 14.0s[1]
Declination	−7° 43′ 07″[1]
Redshift	663 ± 4 km/s[1]
Distance	31.6 ± 1.3 Mly (9.7 ± 0.4 Mpc)[2]
Apparent magnitude (V)	9.9[1]
Characteristics
Type	S0−[3]
Apparent size (V)	7′.2 × 2′.5[1]
Other designations
Spindle Galaxy, UGCA 199, PGC 29265,[1] Caldwell 53

Star formation

NGC 3115 has consumed most of the gas of its youthful accretion disk. It has very little gas and dust left that would trigger new star formation. The vast majority of its component stars are very old.

Black hole

In 1992 John Kormendy of the University of Hawaii and Douglas Richstone of the University of Michigan announced what was observed to be a supermassive black hole in the galaxy.[6] Based on orbital velocities of the stars in its core, the central black hole has mass measured to be approximately one billion solar masses (M_☉). The galaxy appears to have mostly old stars and little or no activity. The growth of its black hole has also stopped.

In 2011, NASA's Chandra X-ray Observatory examined the black hole at the center of the large galaxy. A flow of hot gas toward the supermassive black hole has been imaged, making this the first time clear evidence for such a flow has been observed in any black hole. As gas flows toward the black hole, it becomes hotter and brighter. The researchers found the rise in gas temperature begins at about 700 light years from the black hole, giving the location of the Bondi radius. This suggests that the black hole in the center of NGC 3115 has a mass of about two billion M_☉, supporting previous results from optical observations. This would make NGC 3115 the nearest billion-solar-mass black hole to Earth.

See also

• NGC 5866 – another lenticular galaxy sometimes referred to as the Spindle Galaxy

References

External links

Wikimedia Commons has media related to NGC 3115.

• Chandra Press Release
• SEDS: NGC 3115
• NGC 3115 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images

На других языках

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[de] NGC 3115

NGC 3115 ist eine linsenförmige Galaxie vom Hubble-Typ S0 im Sternbild Sextant südlich der Ekliptik. Sie ist schätzungsweise 22 Millionen Lichtjahre von der Milchstraße entfernt und hat einen Durchmesser von etwa 60.000 Lichtjahre. Das Zentrum der Galaxie beherbergt ein extrem massereiches Schwarzes Loch von etwa zwei Milliarden Sonnenmassen, bei einer Gesamtmasse zwischen 300 und 400 Milliarden Sonnenmassen.[3][4]

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- [en] NGC 3115

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[es] NGC 3115

NGC 3115 o Galaxia de Spindle es una galaxia lenticular en la constelación de Sextans a 32 millones de años luz de distancia. Fue descubierta el 22 de febrero de 1787 por el astrónomo William Herschel.

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[ru] NGC 3115

NGC 3115 (другие обозначения — MCG −1-26-18, UGCA 199, PGC 29265) — галактика в созвездии Секстант на расстоянии 32 миллионов световых лет от нас.

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