PSR 0656+14: X-radiation, geometry and implications of cooling

Details PSR 0656+14: X-radiation, geometry and implications of cooling PSR 0656+14: X-radiation, geometry and implications of cooling

Jan 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994cha%26a..18...49d&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 18, Issue 1, p. 49-53.

Astronomy and Astrophysics

Astrophysics

Neutron Star, X Emission, Geometric Effects

Scientific paper

From an analysis of radio and X observations of PSR 0656+14, we found its rotation axis to be inclined at 30° to its magnetic axis and at 14° to the line of sight. These values will make the theoretical X light curve coincide with the observed curve by the ROSAT satellite. According to the cooling processes in neutron stars and strange stars we found that PSR 0656+14 may either be a proton-rich neutron star (in which direct URCA processes are present) or a strange star.

Affiliated with

Also associated with

No associations

Rating

PSR 0656+14: X-radiation, geometry and implications of cooling 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 PSR 0656+14: X-radiation, geometry and implications of cooling, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and PSR 0656+14: X-radiation, geometry and implications of cooling will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-867019