Changing parameters along the path to the VELA pulsar

Details Changing parameters along the path to the VELA pulsar Changing parameters along the path to the VELA pulsar

May 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985mnras.214p...5h&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 214, May 1, 1985, p. 5P-8P. Research supported by the R

Astronomy and Astrophysics

Astronomy

22

Linear Polarization, Polarization Characteristics, Pulsars, Stellar Rotation, Stellar Spectrophotometry, Polarimeters, Surface Acoustic Wave Devices

Scientific paper

Recent observations of the Vela pulsar, PSR 0833-45, confirm that the
rotation measure of the source is increasing, and show that at the same
time the dispersion measure is decreasing. The observations are
interpreted in terms of a magnetized cloud moving out of the
line-of-sight to the source.

Affiliated with

Also associated with

No associations

Rating

Changing parameters along the path to 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 Changing parameters along the path to the VELA pulsar, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Changing parameters along the path to the VELA pulsar will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1632922