Spectra of short-period pulsars in light of the hypothesis of two types of pulsars

Details Spectra of short-period pulsars in light of the hypothesis of two types of pulsars Spectra of short-period pulsars in light of the hypothesis of two types of pulsars

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985azh....62..608m&link_type=abstract

(Astronomicheskii Zhurnal, vol. 62, May-June 1985, p. 608, 609) Soviet Astronomy (ISSN 0038-5301), vol. 29, May-June 1985, p. 35

Astronomy and Astrophysics

Astronomy

5

Pulsars, Radio Emission, Stellar Models, Stellar Radiation, Stellar Spectra, Magnetospheres, Relativistic Effects, Space Plasmas

Scientific paper

It is shown that the absence of a low-frequency turnover in the spectra of PSR 0531 + 21 and 1937 + 21 can be explained if it is assumed that the radio emission is generated near the light cylinder in these PSR. Differences in two other characteristic features of a PSR spectrum, the high-frequency cutoff and the slope of the linear section, for PSR with short and long periods are discussed.

Affiliated with

Also associated with

No associations

Rating

Spectra of short-period pulsars in light of the hypothesis of two types of pulsars 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 Spectra of short-period pulsars in light of the hypothesis of two types of pulsars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectra of short-period pulsars in light of the hypothesis of two types of pulsars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1664034