Detection of optical pulses from the VELA pulsar

Details Detection of optical pulses from the VELA pulsar Detection of optical pulses from the VELA pulsar

Apr 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977natur.266..692w&link_type=abstract

Nature, vol. 266, Apr. 21, 1977, p. 692-694.

Astronomy and Astrophysics

Astronomy

83

Light Emission, Pulsars, Astrometry, Astronomical Photometry, Light Curve, Position (Location), Position Errors, Stellar Spectrophotometry

Scientific paper

Pulsed optical emission was detected from the Vela pulsar PSR 0833-45.
Double pulses were detected from an area which included Lasker's (1976)
star M, and there is some evidence that the star M is the pulsar. The
pulsed emission has a time-averaged blue magnitude of approximately 25.2
min.

Affiliated with

Also associated with

No associations

Rating

Detection of optical pulses from the VELA pulsar does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Detection of optical pulses from the VELA pulsar, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Detection of optical pulses from the VELA pulsar will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1618393