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Auroras on Planets around Pulsars [PDF]
The Astrophysical Journal Letters, 2023 The first extrasolar planets were discovered serendipitously, by finding the slight variation in otherwise highly regular timing of the pulses, caused by the planets orbiting a millisecond pulsar.
Ruchi Mishra +3 more
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Formation of the planet around the millisecond pulsar J1719-1438 [PDF]
Astronomy & Astrophysics, 2012 Context. Recently the discovery of PSR J1719-1438, a 5.8 ms pulsar with a companion in a 2.2 hr orbit, was reported. The combination of this orbital period and the very low mass function is unique. The discoverers, Bailes et al., proposed an ultracompact
Bailes +24 more
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Possibility of Detection of Exomoons with Inclined Orbits Orbiting Pulsar Planets Using the Time-of-Arrival Analysis [PDF]
Advances in Astronomy, 2014 The perturbation caused by planet-moon binarity on the time-of-arrival (TOA) signal of a pulsar with an orbiting planet is derived for the case of the orbit of the planet-moon system inclined of an angle α with respect to the plane of ...
Antonio Pasqua, Khudhair A. Assaf
doaj +2 more sources
Symposium - International Astronomical Union, 1996 A discovery of three terrestrial-mass planets orbiting the millisecond pulsar PSR B1257+12 and a subsequent detection of the predicted effect of gravitational interaction between the two more massive planets confirms that the first extrasolar planetary system has been identified and that pulsars can be successfully used as probes of planetary dynamics.
A. Wolszczan
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Pulsar Planets Are Exceedingly Rare
Eos, 2022 A new survey of hundreds of pulsars could help solve the mystery of why planets exist around these dead stars.
Kimberly Cartier
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X‐Ray Emission from the Planet Pulsar B1257+12 [PDF]
The Astrophysical Journal, 2007 8 pages, 4 figures, emulateapj.sty; accepted for publication in Astrophysical ...
G. G. Pavlov +3 more
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PSR B1828-11: a precession pulsar torqued by a quark planet? [PDF]
, 2006 The pulsar PSR B1828-11 has long-term, highly periodic and correlated variations in both pulse shape and the rate of slow-down. This phenomenon may provide evidence for precession of the pulsar as suggested previously within the framework of free ...
K. Liu, Link, R. X. Xu, Y. L. Yue
core +5 more sources
Planets, Pulsars, And Poetry [PDF]
International Astronomical Union Colloquium, 1990 For many of us in the United States, the majority of our students are in descriptive astronomy classes. And since these classes typically satisfy general education or core curriculum requirements that must be completed by all students, the students can range from those genuinely interested in astronomy to those who are taking the class because “it ...
S. B. Yorka
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Dynamical Model of Pulsar-Planet Systems [PDF]
, 1994 To appear in "Millisecond Pulsars: A Decade of Surprises" (proceedings of Aspen Winter Astrophysics Conference, eds. A. Fruchter, M Tavani and D.
Renu Malhotra
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Phenomenological constraints on accretion of non-annihilating dark matter on the PSR B1257+12 pulsar from orbital dynamics of its planets [PDF]
, 2010 We analytically compute the effects that a mass variation rate \dot M/M of a pulsar may have on the changes \Delta\tau in the times of arrival of its pulses due to test particle companions, and on their orbital dynamics.
Iorio, Lorenzo
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