NGC 3115
Template:Short description Template:Use mdy dates Template:Infobox 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.<ref>Template:Cite book</ref><ref name=1979A&A....74..235M>Template:Cite journal</ref> 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.
One supernova has been observed in NGC 3115: SN 1935B (type and mag. unknown).<ref>Transient Name Server entry for SN 1935B. Retrieved 28 March 2023.</ref><ref>Central Bureau for Astronomical Telegrams list of Supernovae. Retrieved 28 March 2023.</ref>
Star formationEdit
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 holeEdit
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.<ref>Kormendy, J. and Richstone, D. "Evidence for a supermassive black hole in NGC 3115", Astrophysical Journal, Part 1, vol. 393, no. 2, July 10, 1992, p. 559-578.</ref> Based on orbital velocities of the stars in its core, the central black hole has mass measured to be approximately one billion solar masses (Template:Solar mass). 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 Template:Solar mass, supporting previous results from optical observations. This would make NGC 3115 the nearest billion-solar-mass black hole to Earth.
See alsoEdit
- NGC 5866 – another lenticular galaxy sometimes referred to as the Spindle Galaxy
ReferencesEdit
External linksEdit
- Chandra Press Release
- SEDS: NGC 3115Template:WikiSky
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