Puppis A
Event type | Supernova remnant |
---|---|
S | |
Date | 1971 |
Constellation | Puppis |
Right ascension | 08h 24m 07s |
Declination | -42° 59' 48 |
Epoch | J2000 |
Galactic coordinates | l = 260.2°, b = -3.7° |
Distance | 7,000 ly |
Host | Milky Way |
Progenitor | Unknown |
Progenitor type | Unknown |
Colour (B-V) | Unknown |
Notable features | central source: RX J0822-4300. Apparent size: 1° |
Other designations | SNR G260.4-03.4, MRC 0821-428, 3FHL J0822.1-4253e, 2U 0821-42, 3A 0821-427, 3U 0821-42, 4U 0821-42, AJG 6, INTREF 352, MSH 08-4-04, PKS 0822-42, PKS 0822-428, PKS J0824-4259, 2FGL J0823.0-4246, 3FGL J0822.6-4250e, 2FHL J0822.6-4250e |
Related media on Commons | |
Puppis A (Pup A) is a supernova remnant (SNR) about 100 light-years in diameter and roughly 6500–7000 light-years distant.[1] Its apparent angular diameter is about 1 degree.[2] The light of the supernova explosion reached Earth approximately 3700 years ago. Although it overlaps the Vela Supernova Remnant, it is four times more distant.
A hypervelocity neutron star known as the Cosmic Cannonball has been found in this SNR.
Puppis X-1
Puppis X-1 (Puppis A) was discovered by a Skylark flight in October 1971, viewed for 1 min with an accuracy ≥ 2 arcsec,[3] probably at 1M 0821-426, with Puppis A (RA 08h 23m 08.16s Dec -42° 41′ 41.40″) as the likely visual counterpart.
Puppis A is one of the brightest X-ray sources in the X-ray sky. Its X-ray designation is 2U 0821-42.
Gallery
- Puppis A: X-ray [blue:0.3-8 keV] + IR [red-green:24-70 microns] (21 August 2014).
- Puppis A: X-ray [blue:high]/[green:medium]/[red:low] (10 September 2014).
References
- ^ "Puppis A". WISE Multimedia Gallery. NASA. 9 Dec 2011. Retrieved 21 Nov 2014.
- ^ Milne, D. K. (1971). "Radio observations of the supernova remnants IC443 and Puppis A". Aust. J. Phys. 24: 429. Bibcode:1971AuJPh..24..429M. doi:10.1071/PH710429 (inactive 1 November 2024).
{{cite journal}}
: CS1 maint: DOI inactive as of November 2024 (link) - ^ Wiggin M (December 2000). "The Dome on Ball Hill – The RAE Observatory" (PDF). Archived from the original (PDF) on 2012-02-27.
- "Puppis A: Chandra Reveals Cloud Disrupted By Supernova Shock", Chandra: NASA/CXC/GSFC/U.Hwang et al.; ROSAT: NASA/GSFC/S.Snowden et al., [1]
- Simbad
See also