Classical and general relativistic post-Keplerian effects in binary pulsars hosting fast rotating main sequence stars

We consider a binary system composed of a pulsar and a massive, fast rotating, highly distorted main sequence star of mass M , spin angular momentum S , dimensionless mass quadrupole moment J 2 , equatorial and polar radii R e , R p , flattening ν ≐ ( R e - R p ) / R e , and ellipticity ε ≐ 1 - R p...

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Bibliographic Details
Published in:	The European physical journal. C, Particles and fields Vol. 79; no. 8; pp. 1 - 12
Main Authors:	Iorio, Lorenzo, Rieutord, Michel, Rozelot, Jean-Pierre, de Souza, Armando Domiciano
Format:	Journal Article
Language:	English
Published:	Berlin/Heidelberg Springer Berlin Heidelberg 01.08.2019 Springer Springer Nature B.V Springer Verlag (Germany) SpringerOpen
Subjects:	Analysis Angular momentum Astronomy Astrophysics Astrophysics and Cosmology Binary stars Dipoles Electric waves Electromagnetic radiation Electromagnetic waves Elementary Particles Ellipticity General Relativity and Quantum Cosmology Gravitational fields Gravity Hadrons Heavy Ions Main sequence stars Measurement Science and Instrumentation Millisecond pulsars Nuclear Energy Nuclear Physics Orbits Physics Physics and Astronomy Quadrupoles Quantum Field Theories Quantum Field Theory Regular Article - Theoretical Physics Stellar rotation String Theory Time lag Wave propagation
ISSN:	1434-6044, 1434-6052
Online Access:	Get full text
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