The K-P relation and estimation of emission beam widths for radio pulsars.

Details The K-P relation and estimation of emission beam widths for radio pulsars. The K-P relation and estimation of emission beam widths for radio pulsars.

Jan 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995acaps..15...40w&link_type=abstract

Acta Astrophys. Sin., Vol. 15, No. 1, p. 40 - 46

Astronomy and Astrophysics

Astrophysics

1

Pulsars: Polar Caps, Pulsars: Periods

Scientific paper

The relation between emission beam with (ρ) and period (P) of pulsars is studied via the relation of K-P. The value of K can be easily deduced from observational parameters and is a result by combining the magnetic inclinations with emission beam widths. The values of emission beam width and magnetic inclination are estimated by the new relation between ρ-P and K.

Affiliated with

Also associated with

No associations

Rating

The K-P relation and estimation of emission beam widths for radio 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 The K-P relation and estimation of emission beam widths for radio pulsars., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The K-P relation and estimation of emission beam widths for radio pulsars. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1818051