RX J1242−11
| RX J1242−11 | |
|---|---|
 A Chandra X-ray Observatory image of RX J1242-11. | |
| Observation data (J2000 epoch) | |
| Constellation | Virgo |
| Right ascension | 12h 42m 36.9s |
| Declination | −11° 19′ 35″ |
| Distance | 650 Mly (200 Mpc)[1] |
| Apparent magnitude (V) | c. +14 m |
| Characteristics | |
| Type | elliptical |
| Notable features | Pair of Galaxies = [KG99] A + [KG99] B. |
| Other designations | |
| RX J1242.6-1119A | |
References: 2MASS J12423854-1119207 | |
RX J1242.6−1119A (often abbreviated RX J1242−11) is an elliptical galaxy located approximately 200 megaparsecs (about 650 million light-years) from Earth.
According to current interpretations of X-ray observations made by the Chandra X-ray Observatory and XMM-Newton, the center of this galaxy is a 100 million solar mass supermassive black hole which was observed to have tidally disrupted a star (in 1992 or shortly before).[1] The discovery is widely considered to be the first strong evidence of a supermassive black hole ripping apart a star and consuming a portion of it.[2]
Location in the sky
[edit]The location of RX J1242.6-1119A, as seen from Earth, is less than one degree to the northeast of Messier 104, the Sombrero Galaxy.
References
[edit]- ^ a b Komossa, S.; Halpern, J.; Schartel, N.; Hasinger, G.; Santos-Lleo, M.; Predehl, P. (May 2004), "A Huge Drop in the X-Ray Luminosity of the Nonactive Galaxy RX J1242.6-1119A, and the First Postflare Spectrum: Testing the Tidal Disruption Scenario", The Astrophysical Journal Letters, 603 (1): L17 – L20, arXiv:astro-ph/0402468, Bibcode:2004ApJ...603L..17K, doi:10.1086/382046, S2CID 53724998
- ^ NASA: "Giant Black Hole Rips Apart Unlucky Star"
External links
[edit]
Media related to RX J1242-11 at Wikimedia Commons
- Komossa's Object
- Chandra X-Ray Observatory Photo Album – February 18, 2004
- Auchettl, Katie; Guillochon, James; Ramirez-Ruiz, Enrico (4 April 2017). "New Physical Insights about Tidal Disruption Events from a Comprehensive Observational Inventory at X-Ray Wavelengths". The Astrophysical Journal. 838 (2): 149. doi:10.3847/1538-4357/aa633b.