Note: this is
an archived version which has been superseded. The current SNR
catalogue is at 
https://www.mrao.cam.ac.uk/surveys/snrs/
G263.9−3.3
ADS: search fulltext or
 title/keyword/abstract
 Vela (XYZ)
- Right Ascension: 08 34 00 
 - Declination: −45 50
 - Size (/arcmin): 255 
 - Type: C
 - Flux density at 1 GHz (/Jy): 1750 
 - Spectral Index: varies
 
Notes: This refers to the whole Vela XYZ complex, of which X has at times been classified as a separate (filled-centre) remnant. This remnant is overlapped by G260.4−3.4 and G266.2−1.2.
- Radio: Large shell, with flatter spectrum component (Vela X), and pulsar nebula.
 
- Optical: Filaments.
 
- X-ray: Patchy shell, with extensions, central nebula and pulsar.
 
- Point sources: Pulsar within Vela X, with one-sided `jet'.
 
- Distance: Vela pulsar parallax gives 0.3 kpc, optical spectra and HI studies suggest 0.25 kpc.
 
References:
- Milne 1968, AuJPh, 21, 201. Parkes 64-m at various frequencies, including 408 MHz (48': S=2300±300 Jy), 635 MHz (31': S=2360±300 Jy), 1410 MHz (14': S=1640±300 Jy) and 2650 MHz (7.'5: S=1400±250 Jy), plus discussion of the distance.
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 - Milne 1980, A&A, 81, 293. Maps of Vela X with Parkes 64-m at 1.66, 2.7 and 5 GHz (12', 8.'4 and 4.'4).
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 - Weiler & Panagia 1980, A&A, 90, 269. Clarification of notation of this region and review previous observations.
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 - Bignami & Caraveo 1988, ApJ, 325, L5. Pulsar proper motion from optical observations.
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 - Dwarakanath 1991, JApA, 12, 199. Gauribidanur `T' array at 34.5 MHz (26'×84': S=1800 Jy for Vela X and S=3900 Jy for Vela YZ), plus review of flux densities.
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 - Bietenholz et al. 1991, ApJ, 376, L41. VLA at 5 GHz in vicinity of pulsar.
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 - Willmore et al. 1992, MNRAS, 254, 139. Hard X-ray observations.
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 - Dubner et al. 1992, A&AS, 96, 505. Argentine 30-m at 1.4 GHz (30') of surrounding HI.
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 - Strom et al. 1995, Nature, 373, 590. Radio of X-ray extensions.
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 - Markwardt & Ögelman 1995, Nature, 375, 40. X-ray jet from pulsar.
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 - Jenkins & Wallerstein 1995, ApJ, 440, 227. Optical absorption of associated neutral carbon cloud.
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 - Milne 1995, MNRAS, 277, 1435. Parkes 64-m at 8.4 GHz (3'), including polarisation, of Vela X.
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 - Danks & Sembach 1995, AJ, 109, 2627. Optical spectroscopy of background stars.
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 - Blair et al. 1995, AJ, 110, 312. UV spectroscopy.
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 - Duncan et al. 1996, MNRAS, 280, 252. Parkes 64-m at 2.4 GHz (8.'9).
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 - Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×62'') of part.
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 - Green et al. 1997, AJ, 114, 2058. Parkes 64-m and ATCA OH observations.
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 - Frail et al. 1997, ApJ, 475, 224. VLA at 330 MHz (1'×1.'8) and comparison with ROSAT observations of Vela X.
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 - Markwardt & Ögelman 1997, ApJ, 480, L13. ASCA observations of pulsar `jet'.
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 - Raymond et al. 1997, ApJ, 482, 881. UV spectroscopy.
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 - Yoshikoshi et al. 1997, ApJ, 487, L65. γ-ray observations of pulsar.
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 - Jenkins et al. 1998, ApJ, 492, L147. UV absorption to background star.
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 - Dubner et al. 1998, AJ, 116, 813. Parkes 64-m at 1.4 GHz (15') for HI studies.
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 - Bock et al. 1998, AJ, 116, 1886. MOST at 843 MHz (43''×60'').
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 - Cha et al. 1999, ApJ, 515, L25. Optical spectra, for distance.
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 - Lu & Aschenbach 2000, A&A, 362, 1083. ROSAT spatially resolved spectroscopy.
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 - Chadwick et al. 2000, ApJ, 537, 414. Limit on high energy γ-rays from pulsar.
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 - Sankrit et al. 2001, ApJ, 549, 416. Far-UV observations of selected region.
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 - Pavlov et al. 2001, ApJ, 554, L189. Chandra two epoch observations of pulsar nebula.
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 - Helfand et al. 2001, ApJ, 556, 380. Chandra observations of pulsar and its nebula.
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 - Miyata et al. 2001, ApJ, 559, L45. Chandra of X-ray extension.
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 - Alvarez et al. 2001, A&A, 372, 636. Radio spectral index studies.
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also see: Alvarez et al. 2001, A&A, 379, 323. Erratum.
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 - Caraveo et al. 2001, ApJ, 561, 930. HST parallax observations of pulsar.
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 - Moriguchi et al. 2001, PASJ, 53, 1025. CO observations.
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 - Dodson et al. 2003, MNRAS, 343, 116. ATCA at 1.4, 2.4, 5.2 and 8.5 GHz (6.''2×8.''1, 26''×36'', 10.''5×12.''1 and 10.''6×11.''2) of pulsar nebula.
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 - Sankrit et al. 2003, ApJ, 589, 242. Optical nebulosity to NE of G266.2−1.2.
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 - Nichols & Slavin 2004, ApJ, 610, 285. UV absorption toward background sources.
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 - Hales et al. 2004, ApJ, 613, 977. Vela X at 31 GHz (4.'1).
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 - Mongano et al. 2005, A&A, 436, 917. XMM-Newton and other X-ray observations of pulsar nebula.
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 - Miceli et al. 2005, A&A, 442, 513. XMM-Newton observations of N rim.
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 - Katsuda & Tsunemi 2005, PASJ, 57, 621. XMM-Newton observations of E.
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 - Aharonian et al. 2006, A&A, 448, L43. H.E.S.S. observations.
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 - McConnell et al. 2006, AJ, 131, 648. ATCA at 4.9 GHz (12') including polarisation.
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 - Katsuda & Tsunemi 2006, ApJ, 642, 917. XMM-Newton observations of NE.
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 - Nishikida et al. 2006, ApJ, 644, L171. Far UV observations.
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 - Miceli et al. 2008, ApJ, 676, 1064. XMM-Newton observations.
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 - LaMassa et al. 2008, ApJ, 689, L121. XMM-Newton observations of Vela X.
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 - Grondin et al. 2013, ApJ, 774, 110. Fermi observations of Vela X.
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 - Planck Collaboration: Arnaud et al. 2016, A&A, 586, A134. Planck flux densities at 30, 44 and 70 GHz.
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 - Rao et al. 2016, MNRAS, 455, 2529. Time variation of optical line absorption.
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 - H.E.S.S. Collaboration: Abdalla et al. 2018, A&A, 612, A1. H.E.S.S. observations of Vela X.
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 - Ogbodo et al. 2020, MNRAS, 493, 199. OH maser observations.
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 - Kameswara Rao et al. 2020, MNRAS, 493, 497. Time variation of optical absorption to background stars.
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 - Sapienza et al. 2021, A&A, 649, A56. XMM-Newton observations of clump in SW.
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Last updated: 16 Dec 2022
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