Hercules X-1 pulse profile simulation

Details Hercules X-1 pulse profile simulation Hercules X-1 pulse profile simulation

Jun 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26a...286..497p&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 286, no. 2, p. 497-500

Astronomy and Astrophysics

Astronomy

5

Neutron Stars, Pulsars, Pulse Amplitude, Pulse Duration, Pulsed Radiation, X Ray Astronomy, X Ray Binaries, Accretion Disks, Stellar Magnetic Fields, Stellar Magnetospheres

Scientific paper

We performed calculations of the average X-ray pulse profile observed from the X-ray pulsar Hercules X-1 at the 'main-on' state of the 35-day cycle. We assume that accretion in this source takes place in three distinct zones on the neutron star surface: two magnetic poles and a circle-like area around the pole with lower magnetic field strength, which is connected with a complex (presumably quadrupole) structure of the neutron star magnetic field at its surface.

Affiliated with

Also associated with

No associations

Rating

Hercules X-1 pulse profile simulation 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 Hercules X-1 pulse profile simulation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Hercules X-1 pulse profile simulation will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1862144