Astronomy and Astrophysics – Astronomy
Scientific paper
Nov 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.296..551n&link_type=abstract
In ESA, The 23rd ESLAB Symposium on Two Topics in X Ray Astronomy. Volume 1: X Ray Binaries p 551-556 (SEE N90-25711 19-89)
Astronomy and Astrophysics
Astronomy
Deflection, Light Beams, Neutron Stars, Relativistic Effects, X Ray Astronomy, Bending, Pulse Amplitude, Relativity, Stellar Gravitation, Stellar Mass Accretion, Stellar Radiation
Scientific paper
The deflection of light ray emitted on or near the surface of a neutron star is investigated. A picture of the star as it would appear on a screen far away from the star is computed, giving an impression of the effects of light bending. This geometrical data is combined with emission models in order to obtain frequency dependent pulse shapes. They are compared to the pulse shapes as they would turn out in flat space-time. Relativistic light bending generally tends to flatten the pulse shapes, but in certain cases a new peak may appear, which is totally absent in the non-relativistic case.
Herold Heinz
Kraus Ute
Maile T.
Nollert Hans-Peter
Rebetzky A.
No associations
LandOfFree
Relativistic light bending near neutron stars 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 Relativistic light bending near neutron stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Relativistic light bending near neutron stars will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1614782