Kinematic Projecting of Pulsar Profiles

dc.creatorBordovitqsyn, V. A.
dc.creatorEpp, V. Ya.
dc.creatorBulenok, V. G.
dc.date2001-01-11
dc.date.accessioned2026-07-25T18:01:33Z
dc.descriptionWe suggest a technique for construction of profiles of incoherent pulsar emission using instantaneous angular distribution indicatrix of radiation from relativistic source moving in the neutron star magnetosphere. In the general case the indicatrix depends on the kinematic parameters of radiation source such as velocity and acceleration. The method is illustrated by calculation of the profiles of pulsar radiation based on synchrotron radiation indicatrix. This technique can be easily generalized for the case of other types of relativistic particles radiation. The considered profiles are compared with observed ones. A good agreement was found with profiles of gamma-pulsars - Geminga, Crab and Vela.
dc.descriptionTo be published in proceedings of the 9th Lomonosov Conference on Elementary Particle Physics, Moscow. 10 pages, Latex, 6 eps-figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0101180
dc.identifierhttp://arxiv.org/abs/astro-ph/0101180
dc.identifier.urihttps://dspace.dare.co.zw/handle/123456789/52914
dc.subjectAstrophysics
dc.titleKinematic Projecting of Pulsar Profiles
dc.typetext

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