Vela Pulsar

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Vela Pulsar
Vela Pulsar jet.jpg
The Vela Pulsar and its surrounding pulsar wind nebula, Chandra X-Ray image
Observation data
Epoch J2000      Equinox J2000
Constellation Vela
Right ascension 08h 35m 20.65525s
Declination -45° 10′ 35.1545″[1]
Apparent magnitude (V) 23.6
Astrometry
Distance 959 (-163,+248) ly
(294 (-50,+76)[2] pc)
Other designations
PSR B0833-45, 4U 0833-45, 2CG 263-02, 2E 0833.6-4500, 3EG J0834-4511, H 0833-450, INTEGRAL1 5, SNR G263.6-02.8

The Vela Pulsar (PSR B0833-45 or PSR J0835-4510) is a radio, optical, X-ray and gamma-emitting pulsar associated with Vela Supernova Remnant, in the constellation of Vela.

Contents

Supernova origins [edit]

The association of the Vela pulsar with the Vela Supernova Remnant, made by astronomers at the University of Sydney in 1968,[3] was direct observational proof that supernovae form neutron stars.

Characteristics [edit]

It has a period of 89 milliseconds (the shortest known at the time of its discovery) and the remnant from the supernova explosion is estimated to be travelling at 1,200 km/s (750 mi/s).[4] It has the third brightest optical component of all known pulsars (V = 23.6 mag)[5] which pulses twice for every single radio pulse. The Vela pulsar is the brightest persistent object in the high energy gamma ray sky.

Vela X confusion [edit]

Note that this object has often been called Vela X, for reasons that appear historically unclear. Because of the possible confusion with Vela X-1, a very different kind of object that happens to lie nearby, referring to it as either "Vel X" or "Vela X" seems inadvisable.

Gallery [edit]

Cycle of pulsed gamma rays from the Vela pulsar 
Position of the Vela Pulsar in the Milky Way 
Video of Vela's particle jet 

References [edit]

  1. ^ "Vela pulsar". SIMBAD. Retrieved 9 January 2013. 
  2. ^ Caraveo, P A; De Luca, A; Mignani, R P; Bignami, G F (10 November 2001). "The Distance to the Vela Pulsar Gauged with Hubble Space Telescope Parallax Observations". Astrophys. J. 561 (2): pp. 930–937. doi:10.1086/323377. 
  3. ^ Large, M I; Vaughan, A E; Mills, B Y (26 October 1968). "A Pulsar Supernova Association?". Nature 220 (5165): pp. 340–341. Bibcode:1968Natur.220..340L. doi:10.1038/220340a0. 
  4. ^ Lyne, Andrew G; Graham-Smith, Francis (1998). Pulsar Astronomy (2nd ed.). Cambridge University Press. ISBN 0-521-59413-8. 
  5. ^ Mignani, R P; Zharikov, R P; Caraveo, P A (1 October 2007). "The optical spectrum of the Vela pulsar". Astronomy & Astrophysics 473 (3): p. 891. arXiv:0707.2036. Bibcode:2007A&A...473..891M. doi:10.1051/0004-6361:20077774. 

External links [edit]


Coordinates: Sky map 08h 35m 20.65525s, −45° 10′ 35.1545″