460:
2202:
444:
281:
37:
295:
Vela is the brightest pulsar (at radio frequencies) in the sky and spins 11 times per second (i.e. a period of 89.33 millisecondsâthe shortest known at the time of its discovery) and the remnant from the supernova explosion is estimated to be travelling outwards at 1,200 km/s (750 mi/s). It
335:
Statistically, nearly the 1% of the long-term spin-down of the pulsar is reversed in spin-up glitches, a fraction that is also observed in other monitored pulsars. Careful estimation of the glitch activity and its uncertainty requires statistical tools beyond the simple linear regression.
472:
762:
The H.E.S.S. Collaboration; Aharonian, F.; Benkhali, F. Ait; Aschersleben, J.; Ashkar, H.; Backes, M.; Martins, V. Barbosa; Batzofin, R.; Becherini, Y.; Berge, D.; Bernlöhr, K.; Bi, B.; Böttcher, M.; Boisson, C.; Bolmont, J.; et al. (5 October 2023).
812:
The H.E.S.S. Collaboration; Aharonian, F.; Benkhali, F. Ait; Aschersleben, J.; Ashkar, H.; Backes, M.; Martins, V. Barbosa; Batzofin, R.; Becherini, Y.; Berge, D.; Bernlöhr, K.; Bi, B.; Böttcher, M.; Boisson, C.; Bolmont, J. (5 October 2023).
476:
473:
475:
296:
has the third-brightest optical component of all known pulsars (V = 23.6 mag) which pulses twice for every single radio pulse. The Vela pulsar is the brightest persistent object in the high-energy gamma-ray sky.
648:
325:) large enough to see individual pulses. This observation showed that the pulsar nulled (i.e. did not pulse) for one pulse, with the pulse prior being very broad and the two following pulses featuring low
318:
are sudden spin-ups in the rotation of pulsars. Vela is the best known of all the glitching pulsars, with glitches occurring on average every three years. Glitches are currently not predictable.
443:
2244:
514:
474:
1456:
1202:
Kellogg, E.; Tananbaum, H.; Harnden, F. R. Jr.; Gursky, H.; Giacconi, R.; Grindlay, J. (August 1973). "The X-ray
Structure of the Vela X Region Observed from
909:
Palfreyman, J.; Dickey, J. M.; Hotan, A.; Ellingsen, S.; van
Straten, W. (April 2018). "Alteration of the magnetosphere of the Vela pulsar during a glitch".
867:
Antonelli, Marco; Montoli, Alessandro; Pizzochero, Pierre (November 2022), "Insights into the
Physics of Neutron Star Interiors from Pulsar Glitches",
459:
1365:
1336:
894:
393:, but this phenomenon is separate from either the pulsar or the Vela X nebula. A radio survey of the Vela-Puppis region was made with the
329:. It also appeared that the glitch process took under five seconds to occur and allowed to estimate physical properties of the pulsar.
1449:
687:
1426:
397:
in 1956â57 and identified three strong radio sources: Vela X, Vela Y, and Vela Z. These sources are observationally close to the
322:
321:
On 12 December 2016, Vela was observed to glitch live for the first time with a radio telescope (the 26 m telescope at the
56:
377:
was used to describe the entirety of the supernova remnant. Weiler and
Panagia established in 1980 that Vela X was actually a
2234:
2205:
1442:
1278:
332:
On 22 July 2021, a new glitch occurred. As a result, the period of the pulsar decreased by about 1 part in a million.
1871:
1422:
1245:
709:
679:
1561:
1481:
1208:
596:
Spolon, A.; Zampieri, L.; Burtovoi, A.; Naletto, G.; Barbieri, C.; Barbieri, M.; Patruno, A.; Verroi, E. (2019).
544:
19:
This article is about pulsar associated with the Vela supernova remnant. For high-mass X-ray binary system, see
2239:
373:
spacecraft in 1970â71 showed the Vela pulsar and Vela X to be separate but spatially related objects. The term
538:; De Luca, A.; Mignani, R. P.; Bignami, G. F. (November 2001). "The Distance to the Vela Pulsar Gauged with
2130:
1822:
409:
345:
253:
1991:
1659:
1476:
394:
1465:
1324:
1287:
1254:
1217:
1168:
920:
728:
656:
619:
562:
504:
349:
261:
228:
191:
125:
69:
1649:
2224:
704:
535:
326:
1891:
598:"Timing analysis and pulse proïŹle of the Vela pulsar in the optical band from Iqueye observations"
1184:
1109:
996:
963:
944:
872:
826:
776:
744:
718:
609:
578:
552:
378:
315:
101:
42:
985:"Bayesian estimate of the superfluid moments of inertia from the 2016 glitch in the Vela pulsar"
2185:
1500:
1361:
1332:
1328:
1157:
Large, M. I.; Vaughan, A. E.; Mills, B. Y. (October 1968). "A Pulsar
Supernova Association?".
1139:
1096:
Montoli, Alessandro; Antonelli, Marco; Haskell, Brynmor; Pizzochero, Pierre (5 January 2021).
1078:
1016:
983:
Montoli, Alessandro; Antonelli, Marco; Magistrelli, Fabio; Pizzochero, Pierre (October 2020).
936:
890:
844:
794:
683:
381:, contained within the fainter supernova remnant and driven by energy released by the pulsar.
368:
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207:
187:
52:
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300:
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1291:
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924:
660:
623:
566:
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1527:
815:"Discovery of a radiation component from the Vela pulsar reaching 20 teraelectronvolts"
765:"Discovery of a radiation component from the Vela pulsar reaching 20 teraelectronvolts"
170:
2218:
1522:
1517:
1508:
1317:
1034:
V. Sosa-Fiscella; E. Zubieta; S. del
Palacio; F. Garcia; et al. (23 July 2021).
962:
Ashton, G. (2019). "Rotational evolution of the Vela pulsar during the 2016 glitch".
814:
764:
582:
421:
257:
64:
1188:
748:
1980:
1922:
1644:
1243:
Weiler, K. W.; Panagia, N. (October 1980). "Vela X and the
Evolution of Plerions".
948:
357:
1035:
1011:
984:
740:
2050:
1551:
1542:
1357:
404:
Neither the pulsar nor either of the associated nebulae should be confused with
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288:
90:
886:
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1097:
632:
597:
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Video consisting of eight images of Vela's particle jet, looped continuously
450:
353:
307:
at 1.5 TeV are the only two known pulsar with emission in this energy range
284:
245:
1381:
1058:
940:
1319:
The Cosmic Dance: Science
Discovers the Mysterious Harmony of the Universe
2159:
2120:
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20:
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509:
249:
222:
199:
183:
179:
158:
647:
Manchester, R. N.; Hobbs, G. B.; Teoh, A.; Hobbs, M. (August 2005).
1229:
1114:
1001:
968:
877:
831:
781:
614:
574:
1639:
1389:
723:
401:
supernova remnant, which is also a strong X-ray and radio source.
279:
268:
exploded approximately 11,000â12,300 years ago (and was about 800
241:
195:
1491:
1438:
1036:"A new Glitch in the Vela Pulsar (PSR B0833-45/PSR J0835-4510)"
303:
has been detected from the Vela pulsar and together with the
707:(October 2007). "The Optical Spectrum of the Vela Pulsar".
1059:"PSR1737â30 and period discontinuities in young pulsars"
240:(PSR J0835-4510 or PSR B0833-45) is a radio, optical,
1098:"Statistical estimates of the pulsar glitch activity"
424:
were converted into audible sound by French composer
2176:
2152:
2143:
2108:
2072:
2063:
2023:
1990:
1979:
1913:
1864:
1821:
1658:
1560:
1499:
1490:
869:Astrophysics in the XXI Century with Compact Stars
291:for the pulsar, adapted from Spolon et al. (2019)
674:Lyne, Andrew G.; Graham-Smith, Francis (1998).
16:Multi-spectrum pulsar in the constellation Vela
1450:
515:Centre de données astronomiques de Strasbourg
499:
497:
352:in 1968, was direct observational proof that
95:â45° 10′ 35.1545″
8:
1274:"Radio Emission from the Vela-Puppis Region"
465:Position of the Vela Pulsar in the Milky Way
344:The association of the Vela pulsar with the
2173:
2149:
2069:
1987:
1910:
1496:
1457:
1443:
1435:
389:The pulsar is occasionally referred to as
1299:
1133:
1123:
1113:
1057:McKenna, J.; Lyne, A. G. (January 1990).
1010:
1000:
967:
876:
830:
780:
722:
631:
613:
556:
408:, an observationally close but unrelated
55:J2000
1388:(work details) (in French and English).
2245:Objects with variable star designations
493:
439:
27:
420:The emissions of Vela and the pulsar
7:
862:
860:
858:
41:The Vela Pulsar and its surrounding
1354:Illuminations: Cosmos et esthétique
649:"ATNF Pulsar Catalogue: J0835-4510"
14:
703:Mignani, R. P.; Zharikov, R. P.;
2201:
2200:
1427:NASA/IPAC Extragalactic Database
470:
458:
442:
323:Mount Pleasant Radio Observatory
190: 0833-45, 2CG 263-02,
35:
1272:Rishbeth, H. (December 1958).
1:
1352:Luminet, Jean-Pierre (2011).
1279:Australian Journal of Physics
363:Studies conducted by Kellogg
348:, made by astronomers at the
989:Astronomy & Astrophysics
287:and optical (visible light)
1038:. The Astronomer's Telegram
1012:10.1051/0004-6361/202038340
653:VizieR On-line Data Catalog
2261:
1246:Astronomy and Astrophysics
887:10.1142/9789811220944_0007
841:10.1038/s41550-023-02052-3
791:10.1038/s41550-023-02052-3
741:10.1051/0004-6361:20077774
710:Astronomy and Astrophysics
680:Cambridge University Press
18:
2198:
2172:
1909:
1482:Vela in Chinese astronomy
1472:
1315:Del Re, Giuseppe (2000).
1209:The Astrophysical Journal
933:10.1038/s41586-018-0001-x
299:Pulsed emission up to 20
215:
176:
169:
165:
119:
112:
49:
33:
542:Parallax Observations".
1259:1980A&A....90..269W
1125:10.3390/universe7010008
733:2007A&A...473..891M
102:Apparent magnitude
2131:Vela Supernova Remnant
1872:DENIS J082303.1â491201
540:Hubble Space Telescope
428:and used in the piece
410:high-mass X-ray binary
346:Vela Supernova Remnant
292:
254:Vela Supernova Remnant
1477:List of stars in Vela
1466:Constellation of Vela
633:10.1093/mnras/sty2605
395:Mills Cross Telescope
283:
2235:Vela (constellation)
1923:Gliese 367 b (Tahay)
1877:Gliese 367 (Añañuca)
1360:. pp. 419â420.
1356:(in French). Paris:
1325:Templeton Foundation
871:, pp. 219â281,
453:from the Vela pulsar
350:University of Sydney
252:associated with the
1384:Le Noir de l'Ătoile
1292:1958AuJPh..11..550R
1222:1973ApJ...183..935K
1173:1968Natur.220..340L
925:2018Natur.556..219P
661:2005yCat.7245....0M
624:2019MNRAS.482..175S
567:2001ApJ...561..930C
430:Le noir de l'Ă©toile
327:linear polarization
216:Database references
194: 0833.6-4500,
30:
505:"NAME Vela Pulsar"
379:pulsar wind nebula
340:Research campaigns
293:
210: G263.6-02.8
198: J0834-4511,
182: J0835-4510,
171:Other designations
43:pulsar wind nebula
28:
2212:
2211:
2194:
2193:
2186:Vela Supercluster
2168:
2167:
2139:
2138:
2059:
2058:
1975:
1974:
1905:
1904:
1367:978-2-7381-2562-0
1338:978-1-890151-25-6
1167:(5165): 340â341.
1069:(6256): 349â350.
919:(7700): 219â222.
896:978-981-12-2093-7
825:(11): 1341â1350.
775:(11): 1341â1350.
477:
266:Type II supernova
234:
233:
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2204:
2203:
2174:
2150:
2070:
1988:
1911:
1497:
1459:
1452:
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1401:
1400:
1398:
1396:
1382:"GĂ©rard Grisey:
1378:
1372:
1371:
1349:
1343:
1342:
1323:. Philadelphia:
1322:
1312:
1306:
1305:
1303:
1301:10.1071/PH580550
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1234:
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1181:10.1038/220340a0
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1075:10.1038/343349a0
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819:Nature Astronomy
809:
803:
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784:
769:Nature Astronomy
759:
753:
752:
726:
700:
694:
693:
678:(2nd ed.).
676:Pulsar Astronomy
671:
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558:astro-ph/0107282
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449:Cycle of pulsed
446:
202: 0833-450,
186: B0833-45,
156:
155:
154:
140:
139:
138:
105:
85:
80:
50:Observation data
39:
31:
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2259:
2255:
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2250:
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2240:Optical pulsars
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2190:
2178:Galaxy clusters
2164:
2135:
2104:
2055:
2019:
1982:
1971:
1901:
1860:
1846:85390 (Natasha)
1841:83443 (Kalausi)
1817:
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276:Characteristics
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78:Right ascension
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1892:PSR J0855â4644
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1408:External links
1406:
1403:
1402:
1373:
1366:
1344:
1337:
1307:
1286:(4): 550â563.
1264:
1253:(3): 269â282.
1235:
1230:10.1086/152279
1194:
1149:
1088:
1049:
1026:
975:
954:
901:
895:
854:
804:
754:
717:(3): 891â896.
705:Caraveo, P. A.
695:
688:
666:
639:
608:(1): 175â183.
588:
575:10.1086/323377
551:(2): 930â937.
536:Caraveo, P. A.
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545:Astrophys. J.
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426:GĂ©rard Grisey
423:
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358:neutron stars
355:
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264:. Its parent
263:
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258:constellation
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178:HU Vel,
175:
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65:Constellation
63:
62:
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54:
48:
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38:
32:
26:
22:
1604:
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1510:
1431:
1393:. Retrieved
1386:(1989-1990)"
1383:
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1040:. Retrieved
1029:
992:
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978:
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548:
543:
539:
530:
518:. Retrieved
508:
429:
422:PSR B0329+54
419:
403:
390:
388:
385:Nomenclature
374:
369:
364:
362:
343:
334:
331:
320:
314:
298:
294:
289:light curves
237:
235:
221:
124:
29:Vela Pulsar
25:
2051:Trumpler 10
1423:Vela Pulsar
1414:Vela Pulsar
1358:Odile Jacob
1327:. pp.
1216:: 935â940.
1135:2434/903235
432:(1989â90).
305:Crab pulsar
270:light-years
238:Vela Pulsar
91:Declination
2225:Gum Nebula
2219:Categories
1959:HD 83443 b
1954:HD 85390 b
1949:HD 75289 b
1939:HD 73526 b
1915:Exoplanets
1528:λ (Suhail)
1523:Îș (Markeb)
1115:2012.01539
1002:2005.01594
969:1907.01124
878:2301.12769
832:2310.06181
782:2310.06181
615:1809.07093
488:References
451:gamma rays
354:supernovae
248:-emitting
114:Astrometry
1934:GJ 1132 b
1887:Luhman 16
1144:2218-1997
1083:1476-4687
1021:0004-6361
849:2397-3366
799:2397-3366
724:0707.2036
583:119069765
520:9 January
367:with the
285:Gamma ray
206: 5,
204:INTEGRAL1
104: (V)
2206:Category
2145:Galaxies
2121:HH 46/47
2100:NGC 3132
2095:NGC 2899
2090:NGC 2792
2085:NGC 2736
2080:NGC 2626
1983:clusters
1967:WASP-19b
1813:4293 (i)
1808:4180 (x)
1803:4167 (p)
1798:4143 (t)
1788:4080 (r)
1783:4023 (q)
1778:3990 (Q)
1773:3912 (m)
1768:3836 (M)
1758:3819 (L)
1753:3803 (N)
1748:3753 (I)
1743:3684 (k)
1738:3682 (l)
1733:3614 (c)
1728:3591 (w)
1723:3574 (H)
1713:3520 (g)
1703:3487 (a)
1698:3477 (d)
1693:3452 (n)
1688:3445 (b)
1683:3426 (e)
1678:3407 (C)
1673:3358 (A)
1668:3294 (B)
1590:GP (X-1)
1562:Variable
1545:Tseen Ke
1189:32855796
1108:(1): 8.
1102:Universe
995:: A223.
941:29643483
749:15433523
416:In music
412:system.
406:Vela X-1
399:Puppis A
316:Glitches
311:Glitches
126:Distance
21:Vela X-1
2230:Pulsars
2065:Nebulae
2041:IC 2488
2036:IC 2395
2031:IC 2391
1897:WASP-19
1882:GJ 1132
1288:Bibcode
1255:Bibcode
1218:Bibcode
1169:Bibcode
1042:24 July
949:4708813
921:Bibcode
729:Bibcode
657:Bibcode
620:Bibcode
563:Bibcode
436:Gallery
272:away).
256:in the
57:Equinox
2126:RCW 34
2116:Gum 15
2046:RCW 38
1630:MV (J)
1418:SIMBAD
1395:4 July
1364:
1335:
1187:
1160:Nature
1142:
1081:
1063:Nature
1019:
947:
939:
912:Nature
893:
847:
797:
747:
686:
581:
510:SIMBAD
391:Vela X
375:Vela X
365:et al.
250:pulsar
244:- and
223:SIMBAD
157:
141:
59:J2000
2109:Other
2024:Other
1865:Other
1856:93385
1851:85512
1836:74438
1831:73526
1511:Regor
1501:Bayer
1492:Stars
1390:IRCAM
1331:â25.
1204:Uhuru
1185:S2CID
1110:arXiv
997:arXiv
964:arXiv
945:S2CID
873:arXiv
827:arXiv
777:arXiv
745:S2CID
719:arXiv
610:arXiv
602:MNRAS
579:S2CID
553:arXiv
370:Uhuru
356:form
246:gamma
242:X-ray
108:23.6
53:Epoch
2160:3256
2015:3228
2010:3201
2005:2659
2000:2547
1981:Star
1793:4134
1763:3831
1718:3570
1708:3497
1650:V390
1645:V382
1640:V378
1397:2022
1362:ISBN
1333:ISBN
1140:ISSN
1079:ISSN
1044:2021
1017:ISSN
937:PMID
891:ISBN
845:ISSN
795:ISSN
684:ISBN
522:2013
262:Vela
236:The
229:data
137:â163
135:+248
70:Vela
2153:NGC
2073:NGC
1992:NGC
1543:Ï (
1509:Îł (
1425:at
1416:at
1296:doi
1226:doi
1214:183
1206:".
1177:doi
1130:hdl
1120:doi
1071:doi
1067:343
1007:doi
993:642
929:doi
917:556
883:doi
837:doi
787:doi
737:doi
715:473
628:doi
606:482
571:doi
549:561
301:TeV
260:of
208:SNR
196:3EG
184:PSR
180:PSR
153:â50
151:+76
148:294
132:959
2221::
1823:HD
1660:HR
1635:NX
1625:KQ
1620:IM
1615:HY
1610:HX
1605:HU
1600:GZ
1595:GX
1585:AI
1580:AH
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192:2E
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1930:d
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Text is available under the Creative Commons Attribution-ShareAlike License. Additional terms may apply.
