Unusual properties of the pulsar PSR 1822-09

Details Unusual properties of the pulsar PSR 1822-09 Unusual properties of the pulsar PSR 1822-09

Jan 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26a....93...54f&link_type=abstract

Astronomy and Astrophysics, vol. 93, no. 1-2, Jan. 1981, p. 54-61. Research supported by the Alexander von Humboldt-Stiftung.

Astronomy and Astrophysics

Astrophysics

41

Astrophysics, Pulsars, Stellar Radiation, Gamma Ray Astronomy, Polarized Radiation, Radiant Flux Density, Telescopes

Scientific paper

The pulsar PSR 1822-09 (a suspected gamma-ray source) has been observed at 1620 MHz, 1720 MHz, and 2650 MHz. The emission is found to switch repeatedly between two distinct modes, each with characteristic intensity and subpulse behavior patterns. In the 'quiescent' mode, the first component of the main pulse is extremely weak and a stable, long-period subpulse drift is observed in the second component. In the 'burst' mode, the first component becomes prominent with only occasional short-period drift occurring in the second component. The interpulse emission is detected at 1720 MHz and evidence of its participation in the mode-changing is presented. An attempt is made to account for these observations in terms of current pulsar emission theories.

Affiliated with

Also associated with

No associations

Rating

Unusual properties of the pulsar PSR 1822-09 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 Unusual properties of the pulsar PSR 1822-09, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Unusual properties of the pulsar PSR 1822-09 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1050601