22h 02m 43.3s, +42° 16′ 40″BL Lacertae
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| BL Lacertae | |
|---|---|
| Lua error in package.lua at line 80: module 'Module:InfoboxImage/data' not found. The active galaxy BL Lacertae (center), from the Pan-STARRS Data Release 1. The bright object at the left is a foreground star within the Milky Way. Green pixels are artifacts due to data processing. | |
| Observation data (Epoch J2000) | |
| Constellation | Lacerta |
| Right ascension | Template:RA |
| Declination | Template:DEC |
| Redshift | 0.07 |
| Distance | 0.9 Gly (0.276 Gpc) |
| Type | BL Lac |
| Apparent magnitude (V) | var. ~14 to ~17 |
| Other designations | |
| OY+401, VR 42.22.01 | |
| See also: Quasar, List of quasars | |
BL Lacertae or BL Lac is a highly variable, extragalactic active galactic nucleus (AGN or active galaxy). It was first discovered by Cuno Hoffmeister in 1929,[1] but was originally thought to be an irregular variable star in the Milky Way galaxy and so was given a variable star designation. In 1968, the "star" was identified by John Schmitt at the David Dunlap Observatory as a bright, variable radio source. A faint trace of a host galaxy was also found.[2] In 1974, Oke and Gunn measured the redshift of BL Lacertae as z = 0.07, corresponding to a recession velocity of 21,000 km/s with respect to the Milky Way.[3] The redshift figure implies that the object lies at a distance of 900 million light years.
Due to its early discovery, BL Lacertae became the prototype and namesake of the class of active galactic nuclei known as "BL Lacertae objects" or "BL Lac objects". This class is distinguished by rapid and high-amplitude brightness variations and by optical spectra devoid (or nearly devoid) of the broad emission lines characteristic of quasars. These characteristics are understood to result from relativistic beaming of emission from a jet of plasma ejected from the vicinity of a supermassive black hole. BL Lac objects are also categorized as a type of blazar.
BL Lacertae changes in apparent magnitude over fairly small time periods, typically between values of 14 and 17. In January 2021, it exhibited extreme flaring behavior and was reported to reach magnitude 11.45 in the R filter band.[5]
References
- ^ Page Module:Citation/CS1/styles.css has no content.Hoffmeister, Cuno (1929). "354 neue Veränderliche". Astronomische Nachrichten. 236 (15): 233–244. Bibcode:1929AN....236..233H. doi:10.1002/asna.19292361502.
- ^ Page Module:Citation/CS1/styles.css has no content.Schmitt, John L. (May 1968). "BL Lac identified as a Radio Source". Nature. 218 (5142): 663. Bibcode:1968Natur.218..663S. doi:10.1038/218663a0. S2CID 4213061.
- ^ Page Module:Citation/CS1/styles.css has no content.Oke, J. B.; Gunn, J. E. (1974). "The Distance of BL Lacertae". Astrophysical Journal Letters. 189: 5. Bibcode:1974ApJ...189L...5O. doi:10.1086/181450.
- ^ Page Module:Citation/CS1/styles.css has no content."Download Data". aavso.org. AAVSO. Retrieved 1 October 2021.
- ^ Page Module:Citation/CS1/styles.css has no content.Bonnoli, Giacomo. "ATel #14329". The Astronomer's Telegram. Retrieved 20 January 2021.
External links
- Page Module:Citation/CS1/styles.css has no content."BL Lacertae". aavso.org. 13 April 2010.
- Page Module:Citation/CS1/styles.css has no content."NAME BL Lac". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 3 April 2018.
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