RX J0852.0−4622 or Vela Junior
The purple in this image is a false color indication of the x-rays detected by the Chandra X-Ray Observatory emanating from the edge of the supernova remnant due to a shockwave front. The center of the remnant is out of frame, off to the left.
Event typeSupernova remnant Edit this on Wikidata
SN
Date1998
ConstellationVela
Right ascension08h 52m
Declination−46° 22′
EpochJ2000.0
Galactic coordinates286.9460 +42.4568 (34" W, 10" S)
Distance>1500 ly
RemnantCXOU J085201.4-461753
Notable featurescentral object in SNR RX J0852.0−4622 = AX J0851.9−4617.
Other designationsSNR G266.2-01.2, SNR G266.3-01.2, 3FHL J0851.9-4620e, RX J0852.0-4622, 2FGL J0851.7-4635, 3FGL J0852.7-4631e, 2FHL J0852.8-4631, 2FHL J0852.8-4631e

RX J0852.0−4622 (also known as G266.2−1.2) is a supernova remnant. The remnant is located in the southern sky in the constellation Vela ("sail"), and sits (in projection) inside the much larger and older Vela Supernova Remnant. For this reason, RX J0852.0−4622 is often referred to as Vela Junior (Vela Jr.).[1][2] There have been a minority of suggestions that the remnant may be a spurious identification of a complicated substructure within the larger and better studied Vela SNR, but most studies accept that G266.2−1.2 is a SNR in its own right. Indeed, its detection in the high energy Teraelectronvolt range by the High Energy Stereoscopic System in 2005 is strong confirmation of such.[3]

It was found in 1998 with an analysis of data from the ROSAT x-ray telescope.[4] Published simultaneously with its discovery was a claimed detection by the Compton Gamma Ray Observatory of a gamma ray spectral line of 44Ti which has a half-life of 60 years and therefore seemed to indicate a young provenance for the supernova, perhaps the youngest one yet discovered.[5] Later independent groups could not reproduce the detection, and so the consensus is that the identification of this line was likely spurious.[6] Since the age and distance are correlated, a young, nearby supernova like this has inspired some detective work to identify evidence that such a supernova may have been observed and recorded by groups of people,[7] and geochronologists have looked for evidence of a young supernova in tree ring[8] and ice core data,[9] but identification of claimed correlate signals have not been conclusively made.[2] The latest analyses of the remnant indicate an age of at least 2400 years (and possibly much older), a distance of no less than 500 parsecs, and a radial size of at least 8 parsecs.[2]

The central compact object (CCO) was discovered in 2001.[10] In the initial Chandra X-ray image and deeper images thereafter, no pulsations were detected from the compact remnant, which is believed to be the neutron star CXOU J085201.4-461753. A different pulsar was suggested as the remnant,[11] but its kinematics do not conform as well to the observed kinematics of the remnant shell.[2]

References

  1. ↑ SNRcat: Supernova Remnant G266.2-01.2
  2. 1 2 3 4 Allen, G. E.; Chow, K.; Delaney, T.; Filipović, M. D.; Houck, J. C.; Pannuti, T. G.; Stage, M. D. (2014). "ON THE EXPANSION RATE, AGE, AND DISTANCE OF THE SUPERNOVA REMNANT G266.2–1.2 (Vela Jr.)". The Astrophysical Journal. 798 (2): 82. doi:10.1088/0004-637X/798/2/82. hdl:1721.1/94531. S2CID 11391141.
  3. ↑ Aharonian, F.; Akhperjanian, A. G.; Bazer-Bachi, A. R.; Beilicke, M.; Benbow, W.; Berge, D.; Bernlöhr, K.; Boisson, C.; Bolz, O.; Borrel, V.; Braun, I.; Breitling, F.; Brown, A. M.; Chadwick, P. M.; Chounet, L. -M. (2005-07-01). "Detection of TeV γ-ray emission from the shell-type supernova remnant RX J0852.0-4622 with HESS". Astronomy and Astrophysics. 437 (1): L7–L10. arXiv:astro-ph/0505380. Bibcode:2005A&A...437L...7A. doi:10.1051/0004-6361:200500130. ISSN 0004-6361.
  4. ↑ Aschenbach, B. (1998). "Discovery of a young nearby supernova remnant" (PDF). Nature. 396 (6707): 141–142. Bibcode:1998Natur.396..141A. doi:10.1038/24103. S2CID 4426317.
  5. ↑ Iyudin, A. F.; Schönfelder, V.; Bennett, K.; Bloemen, H.; Diehl, R.; Hermsen, W.; Lichti, G. G.; van der Meulen, R. D.; Ryan, J.; Winkler, C. (1998-11-01). "Emission from 44Ti associated with a previously unknown Galactic supernova". Nature. 396 (6707): 142–144. Bibcode:1998Natur.396..142I. doi:10.1038/24106. ISSN 0028-0836. S2CID 4430526.
  6. ↑ Slane, Patrick; Hughes, John P.; Edgar, Richard J.; Plucinsky, Paul P.; Miyata, Emi; Tsunemi, Hiroshi; Aschenbach, Bernd (2001-02-01). "RX J0852.0-4622: Another Nonthermal Shell-Type Supernova Remnant (G266.2-1.2)". The Astrophysical Journal. 548 (2): 814–819. arXiv:astro-ph/0010510. Bibcode:2001ApJ...548..814S. doi:10.1086/319033. ISSN 0004-637X.
  7. ↑ Aschenbach, B.; Iyudin, A. F.; Schönfelder, V. (1999-10-01). "Constraints of age, distance and progenitor of the supernova remnant RX J0852.0-4622/GRO J0852-4642". Astronomy and Astrophysics. 350: 997–1006. arXiv:astro-ph/9909415. Bibcode:1999A&A...350..997A. ISSN 0004-6361.
  8. ↑ Michelle Starr: The Rings of Ancient Trees May Hold Tales of Epic Space Explosions, on: sciencealert, 14 November 2020
  9. ↑ Burgess, C. P.; Zuber, K. (2000-08-01). "Footprints of the newly discovered Vela supernova in Antarctic ice cores?". Astroparticle Physics. 14 (1): 1–6. arXiv:astro-ph/9909010. Bibcode:2000APh....14....1B. doi:10.1016/S0927-6505(00)00102-X. ISSN 0927-6505. S2CID 6392917.
  10. ↑ Pavlov, G. G.; Sanwal, D.; Kiziltan, B.; Gairmire, G. P. (2001). "The Compact Central Object in the RX J0852.0−4622 Supernova Remnant". The Astrophysical Journal. 559 (2): L131. arXiv:astro-ph/0108150. Bibcode:2001ApJ...559L.131P. doi:10.1086/323975. S2CID 8439326.
  11. ↑ Redman, M. P.; Meaburn, J. (2005-01-01). "A possible association of a young pulsar (PSR J0855-4644) with the young Vela supernova remnant RX J0852.0-4622". Monthly Notices of the Royal Astronomical Society. 356 (3): 969–973. Bibcode:2005MNRAS.356..969R. doi:10.1111/j.1365-2966.2004.08523.x. ISSN 0035-8711.
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