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Dynamics of two planets in the 3/2 mean-motion resonance: Application to the planetary system of the pulsar PSR B1257+12
(Springer, 2006-04-01)
This paper considers the dynamics of two planets, as the planets B and C of the pulsar PSR B1257+12, near a 3/2 mean-motion resonance. A two-degrees-of-freedom model, in the framework of the general three-body planar ...
Dynamics of two planets in the 3/2 mean-motion resonance: Application to the planetary system of the pulsar PSR B1257+12
(Springer, 2006-04-01)
This paper considers the dynamics of two planets, as the planets B and C of the pulsar PSR B1257+12, near a 3/2 mean-motion resonance. A two-degrees-of-freedom model, in the framework of the general three-body planar ...
Evolutionary trajectories of ultracompact "black widow" pulsars with very low mass companions
(IOP Publishing, 2012-07)
The existence of millisecond pulsars with planet-mass companions in close orbits is challenging from the stellar evolution point of view. We calculate in detail the evolution of binary systems self-consistently, including ...
EVOLUTIONARY TRAJECTORIES OF ULTRACOMPACT "BLACK WIDOW" PULSARS WITH VERY LOW MASS COMPANIONS
(IOP PUBLISHING LTDBRISTOL, 2012)
The existence of millisecond pulsars with planet-mass companions in close orbits is challenging from the stellar evolution point of view. We calculate in detail the evolution of binary systems self-consistently, including ...
Rotating ridig bodies, moment of inertia, parallel axis and perpendicular axis theorem, rotational kinetic energy, fly wheels, neutron stars, pulsars
(MIT OpenCourseWare – Massachussetts Institute of Technology, 2011)
Rotating ridig bodies, moment of inertia, parallel axis and perpendicular axis theorem, rotational kinetic energy, fly wheels, neutron stars, pulsars
(MIT OpenCourseWare – Massachussetts Institute of Technology, 2016)
A Low-Mass Planet with a Possible Sub-Stellar-Mass Host in Microlensing Event MOA-2007-BLG-192
(2008)
We report the detection of an extrasolar planet of mass ratio q ~ 2 × 10−4 in microlensing event MOA-2007-BLG-192. The best-fit microlensing model shows both the microlensing parallax and finite source effects, and these ...