Simeis 147
Simeis 147, also known as the Spaghetti Nebula, SNR G180.0-01.7 or Sharpless 2-240, is a supernova remnant (SNR) in the Milky Way, straddling the border between the constellations Auriga and Taurus. Discovered in 1952 at the Crimean Astrophysical Observatory using a 25-inch Schmidt-Cassegrain telescope, it is difficult to observe due to its extremely low brightness.
The supernova remnant nebula from Simeis 147 or the Spaghetti Nebula. | |
Other designations | 3FHL J0537.6+2751e, 2FGL J0538.1+2718, 3FGL J0540.3+2756e, 2FHL J0534.1+2753 |
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Event type | Supernova remnant |
Spectral class | Unknown |
Date | 1952[1] |
Instrument | Crimean Astrophysical Observatory |
Constellation | Taurus |
Right ascension | 05h 39m 06s |
Declination | +27° 59′ 55″ |
Epoch | J2000 |
Galactic coordinates | Unknown |
Distance | 3,000 light-years (0.92 kpc) |
Remnant | Mixed-morphology |
Host | Milky way |
Progenitor | Unknown |
Progenitor type | Unknown |
Colour (B-V) | Unknown |
Peak apparent magnitude | 6.5 |
The nebulous area is fairly large with an almost spherical shell and filamentary structure.[2] The remnant has an apparent diameter of approximately 3 degrees, an estimated distance of approximately 3000 (±350) light-years, and an age of approximately 40,000 years.[3]
It is believed that after its stellar explosion a rapidly spinning neutron star known as pulsar PSR J0538+2817 was left behind in the nebula core, emitting a strong radio signal.[4]
References
- "Simeis 147, Supernova Remnant in Taurus". AstroPix. 28 February 2013.
- "VizieR query result". Centre de Données astronomiques de Strasbourg. 20 December 2013.
- Nemiroff, R.; Bonnell, J., eds. (9 October 2012). "Simeis 147: Supernova Remnant". Astronomy Picture of the Day. NASA.
- "SNR G180.0–01.7". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 20 December 2013.
External links
- VizieR Query
- SIMBAD Query
- APOD NASA 2016 April 25
- APOD NASA 2017 May 18