2013MNRAS.428.2295B


Query : 2013MNRAS.428.2295B

2013MNRAS.428.2295B - Mon. Not. R. Astron. Soc., 428, 2295-2310 (2013/January-3)

A first-order secular theory for the post-Newtonian two-body problem with spin - I. The restricted case.

BISCANI F. and CARLONI S.

Abstract (from CDS):

We revisit the relativistic restricted two-body problem with spin employing a perturbation scheme based on Lie series. Starting from a post-Newtonian expansion of the field equations, we develop a first-order secular theory that reproduces well-known relativistic effects such as the precession of the pericentre and the Lense-Thirring and geodetic effects. Additionally, our theory takes into full account the complex interplay between the various relativistic effects, and provides a new explicit solution of the averaged equations of motion in terms of elliptic functions. Our analysis reveals the presence of particular configurations for which non-periodical behaviour can arise. The application of our results to real astrodynamical systems (such as Mercury-like and pulsar planets) highlights the contribution of relativistic effects to the long-term evolution of the spin and orbit of the secondary body.

Abstract Copyright: © 2012 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2012)

Journal keyword(s): gravitation - celestial mechanics

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 PSR J1719-14 Psr 17 19 10.076221 -14 38 01.00200           ~ 92 2

Query : 2013MNRAS.428.2295B

Basic data :
PSR J1719-14 -- Pulsar
Other object types:
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Psr (PSR)
ICRS coord. (ep=J2000) :
17 19 10.076221 -14 38 01.00200 (Radio) [ 0.05837 0.4 90 ] B 2024MNRAS.530..287S
FK4 coord. (ep=B1950 eq=1950) :
17 16 19.163136 -14 34 57.06546 [ 0.05837 0.4 90 ]
Gal coord. (ep=J2000) :
008.858500313 +12.838322549 [ 0.05837 0.4 90 ]
Proper motions mas/yr :
3.76 -3.3 [0.1 0.5 90] C 2024MNRAS.530..287S
Parallaxes (mas):
0.3 [0.23] C 2024MNRAS.530..287S
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PSR J1719-14 PSR J1719-1438

References (92 between 1850 and 2026) (Total 92)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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