NGC 4526
lenticular galaxy in the constellation Virgo
NGC 4526 is a lenticular galaxy in the Virgo constellation. In a telescope, it looks like a lentil-shaped structure with spiral arms. It is one of the brightest lenticular galaxies.[3] It is thought that a supermassive black hole is in the center of the galaxy. Astronomers say that the supermassive black hole is 450 million times the mass of the Sun.[4]
| NGC 4526 | |
|---|---|
 | |
| Observation data | |
| Constellation | Virgo |
| Right ascension | 12h 34m 03.029s[1] |
| Declination | +07° 41′ 56.90″ |
| Redshift | 0.001494±0.000027 |
| Helio radial velocity | 448±8 km/s |
| Distance | 55±5 Mly (16.9±1.6 Mpc)[2] |
Since astronomers found this galaxy, two supernovas have occurred around it. The most recent was SN 1994D, which was the supernova of a white dwarf that was made of carbon and oxygen. NGC 4526 spins at a speed of 250 kilometers per second (559,234 mph or about 900,000 kph).[5]
References
change- ↑ Skrutskie, M. F.; et al. (February 2006), "The Two Micron All Sky Survey (2MASS)", Astrophysical Journal, 131 (2): 1163–1183, Bibcode:2006AJ....131.1163S, doi:10.1086/498708, S2CID 18913331.
- ↑ Tonry, J. L.; et al. (2001), "The SBF Survey of Galaxy Distances. IV. SBF Magnitudes, Colors, and Distances", Astrophysical Journal, 546 (2): 681–693, arXiv:astro-ph/0011223, Bibcode:2001ApJ...546..681T, doi:10.1086/318301, S2CID 17628238.
- ↑ Burstein, D. (November 1979), "Structure and origin of S0 galaxies. I - Surface photometry of S0 galaxies", Astrophysical Journal Supplement Series, 41: 435–450, Bibcode:1979ApJS...41..435B, doi:10.1086/190625.
- ↑ Davis, Timothy A.; et al. (February 2013), "A black-hole mass measurement from molecular gas kinematics in NGC4526", Nature, 494 (7437): 328–330, arXiv:1301.7184, Bibcode:2013Natur.494..328D, doi:10.1038/nature11819, PMID 23364690, S2CID 205232307.
{{citation}}:|last2=has generic name (help) - ↑ "The whirling disc of NGC 4526". www.spacetelescope.org. ESA/Hubble. Archived from the original on 24 October 2014. Retrieved 20 October 2014.