HOPS 383
Appearance
![](http://upload.wikimedia.org/wikipedia/commons/thumb/8/83/PIA18928-Protostar-HOPS383-20150323.jpg/250px-PIA18928-Protostar-HOPS383-20150323.jpg)
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Orion |
Right ascension | 5h 35m 29.81s |
Declination | −4° 59′ 51.1″ |
Distance | 1,400 ly (420 pc) |
Spectral type | Class 0 protostar |
Other designations | |
HOPS 383 |
HOPS 383 is a Class 0 protostar. It is the first class-0 protostar discovered to have had an outburst,[1] and as of 2020, the youngest protostar known to have had an outburst.[1] The protostar was discovered by the Herschel Orion Protostar Survey (HOPS) team.[2]
Outburst
HOPS 383 had an outburst between 2004 and 2006 (a "dramatic mid-infrared brightening"); the increase in magnitude was detectable at the 24 μm (35 times increase) and 4.5 μm, and was also detectable at the submillimetre.[3] After 6 years, observations showed no signs of fading.[3]
References
- ^ a b "NASA satellites catch 'growth spurt' from newborn protostar". Science Daily. 24 March 2015.
- ^ "NRL Astrophysicist Explores Star Formation in Orion's Belt". U.S. Department of Defense. 6 March 2015.
- ^ a b Safron, Emily J.; Megeath, S. Thomas; Booker, Joseph; Fischer, William J.; Furlan, Elise; Rebull, Luisa M.; Stutz, Amelia M.; Stanke, Thomas; Billot, Nicolas; Tobin, John J.; Ali, Babar (2015-02-10). "HOPS 383: AN OUTBURSTING CLASS 0 PROTOSTAR IN ORION". Astrophysical Journal Letters. 800 (1). doi:10.1088/2041-8205/800/1/L5. ISSN 2041-8205.
Further reading
- "HOPS 383: An Outbursting Class 0 Protostar in Orion"; Emily J. Safron, William J. Fischer, S. Thomas Megeath, Elise Furlan, Amelia M. Stutz, Thomas Stanke, Nicolas Billot, Luisa M. Rebull, John J. Tobin, Babar Ali, Lori E. Allen, Joseph Booker, Dan M. Watson, T. L. Wilson; The Astrophysical Journal Letters, Volume 800, Issue 1, article id. L5, 6 pp. (2015) February 2015; arXiv:1501.00492; Bibcode:2015ApJ...800L...5S; doi:10.1088/2041-8205/800/1/L5;