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...

Celý popis

Uložené v:

Podrobná bibliografia
Vydané v:	The European physical journal. C, Particles and fields Ročník 79; číslo 8; s. 1 - 12
Hlavní autori:	Iorio, Lorenzo, Rieutord, Michel, Rozelot, Jean-Pierre, de Souza, Armando Domiciano
Médium:	Journal Article
Jazyk:	English
Vydavateľské údaje:	Berlin/Heidelberg Springer Berlin Heidelberg 01.08.2019 Springer Springer Nature B.V Springer Verlag (Germany) SpringerOpen
Predmet:	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
On-line prístup:	Získať plný text
Tagy:	Pridať tag Žiadne tagy, Buďte prvý, kto otaguje tento záznam!

Buďte prvý, kto okomentuje tento záznam!