Puppis A

Puppis A
	The Chandra three-color image (inset) is a region of the supernova remnant Puppis A (wide-angle view from ROSAT in blue) which reveals a cloud being torn apart by a shock wave produced in a supernova explosion. ROSAT image is 88 arcmin across; Chandra image 8 arcmin across. RA 08h 23m 08.16s Dec -42° 41′ 41.40″ in Puppis. Observation date: September 4, 2005. Color code: Energy (Red 0.4-0.7 keV; Green 0.7-1.2 keV; Blue 1.2-10 keV). Instrument: ACIS. Credit: Chandra: NASA/CXC/GSFC/U.Hwang et al.; ROSAT: NASA/GSFC/S.Snowden et al.
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
	[edit on Wikidata]

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 08^h 23^m 08.16^s 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.

External links

Media related to Puppis A at Wikimedia Commons

Chandra: Puppis A, date: 10 September 2014, retrieved 4 March 2025
Puppis A: Chandra Reveals Cloud Disrupted By Supernova Shock, Chandra: NASA/CXC/GSFC/U.Hwang et al.; ROSAT: NASA/GSFC/S.Snowden et al.,
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[1] "Puppis A". WISE Multimedia Gallery. NASA. 9 Dec 2011. Retrieved 21 Nov 2014.

[2] 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-3] Wiggin M (December 2000). "The Dome on Ball Hill – The RAE Observatory" (PDF). Archived from the original (PDF) on 2012-02-27.

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Puppis A

Contents

Puppis X-1

Gallery

References

See also

External links

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