NGC 1266
In this article we will explore in detail the fascinating world of NGC 1266, a topic that has sparked the interest and curiosity of people of all ages and backgrounds. From its impact on modern society to its historical relevance, NGC 1266 has left an indelible mark on the world around us. Throughout these pages, we will discover the various facets of NGC 1266, its practical applications and its influence in different fields. Whether you are an expert in the field or are just getting into it, this article will provide you with a complete and enriching overview of NGC 1266. Get ready to embark on a journey of discovery and learning!
| NGC 1266 | |
|---|---|
 Hubble image of NGC 1266 | |
| Observation data (J2000 epoch) | |
| Constellation | Eridanus |
| Right ascension | 03h 16m 00.7s[1] |
| Declination | −02° 25′ 38″[1] |
| Redshift | 0.007238 ± 0.000017[2] |
| Heliocentric radial velocity | 2170 ± 5 km s−1[2] |
| Distance | 29.9 Mpc[2] |
| Characteristics | |
| Type | S0[2] |
| Half-light radius (physical) | 2.96 kpc |
| Half-light radius (apparent) | 20.4"[2] |
| Notable features | AGN, molecular outflow, suppressed SFR |
| Other designations | |
| PGC 12131 | |
NGC 1266 is a lenticular galaxy in the constellation Eridanus. Although not currently starbursting, it has undergone a period of intense star formation in the recent past, ceasing only ≈500 Myr ago.[3] The galaxy is host to an obscured active galactic nucleus.[4]
A massive molecular outflow, with 2.4 × 107 M of hydrogen, is present from the nucleus of the galaxy,[4] at a rate of 110 M yr−1.[5] Less than 2% of the gas (2 M yr−1) is escaping the galaxy. Momentum coupling to the jet of the AGN is likely driving the outflow.[5]
The current observed star-formation rate (SFR) of ~0.87 M yr−1 is significantly lower than expected for a galaxy of its properties, suppressed by a factor of 50 to 150. Authors have put forth several hypotheses to explain these observations. The most likely scenario is that the AGN-driven molecular outflow is injecting turbulence into the nuclear regions, preventing gravitational collapse of molecular clouds.[5] NGC 1266 is the first known intermediate-mass galaxy to show AGN-driven suppression of star formation.
Two hypotheses exist to explain NGC 1266's nuclear activity and excessive far-IR emission. Either a heavily obscured ultracompact starburst is present in the nuclear regions, or a powerful buried AGN is present, beyond what has been inferred from other observations. Neither scenario is without problems. The black hole at the center of the galaxy is likely growing according to the M–sigma relation, and eventually the outflow will result in the removal of the majority of the gas from the nucleus.[5]
References
- ^ a b Paturel, G.; Petit, C.; Prugniel, Ph.; Theureau, G.; Rousseau, J.; Brouty, M.; Dubois, P.; Cambrésy, L. (2003). "HYPERLEDA. I. Identification and designation of galaxies". Astronomy and Astrophysics. 412: 45–55. Bibcode:2003A&A...412...45P. doi:10.1051/0004-6361:20031411.
- ^ a b c d e Cappellari, Michele; Emsellem, Eric; Krajnović, Davor; McDermid, Richard M; Scott, Nicholas; Verdoes Kleijn, G. A; Young, Lisa M; Alatalo, Katherine; Bacon, R; et al. (2011). "The ATLAS3D project - I. A volume-limited sample of 260 nearby early-type galaxies: Science goals and selection criteria". Monthly Notices of the Royal Astronomical Society. 413 (2): 813–836. arXiv:1012.1551. Bibcode:2011MNRAS.413..813C. doi:10.1111/j.1365-2966.2010.18174.x. S2CID 15391206.
{{cite journal}}:|last13=has generic name (help) - ^ Alatalo, Katherine; Nyland, Kristina; Graves, Genevieve; Deustua, Susana; Griffin, Kristen Shapiro; Duc, Pierre-Alain; Cappellari, Michele; McDermid, Richard M; Davis, Timothy A; et al. (2013). "Ngc 1266 As a Local Candidate for Rapid Cessation of Star Formation". The Astrophysical Journal. 780 (2): 186. arXiv:1311.6469. Bibcode:2014ApJ...780..186A. doi:10.1088/0004-637X/780/2/186. S2CID 14612978.
{{cite journal}}:|last19=has generic name (help) - ^ a b Alatalo, K; Blitz, L; Davis, T. A; Bureau, M; Lopez, L. A; Cappellari, M; Scott, N; Shapiro, K. L; Crocker, A. F; et al. (2011). "Discovery of an Active Galactic Nucleus Driven Molecular Outflow in the Local Early-Type Galaxy Ngc 1266". The Astrophysical Journal. 735 (2): 88. arXiv:1104.2326. Bibcode:2011ApJ...735...88A. doi:10.1088/0004-637X/735/2/88. S2CID 19036583.
{{cite journal}}:|last4=has generic name (help) - ^ a b c d Alatalo, Katherine; Lacy, Mark; Lanz, Lauranne; Bitsakis, Theodoros; Appleton, Philip N; Nyland, Kristina; Cales, Sabrina L; Chang, Philip; Davis, Timothy A; et al. (2014). "Suppression of Star Formation in Ngc 1266". The Astrophysical Journal. 798 (1): 31. arXiv:1410.4556. Bibcode:2015ApJ...798...31A. doi:10.1088/0004-637X/798/1/31. S2CID 15747241.
External links
- NGC 1266 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
