No planet orbiting PS R1829–10

  title={No planet orbiting PS R1829–10},
  author={Andrew G. Lyne and Matthew Bailes},
Minerva-Australis. I. Design, Commissioning, and First Photometric Results
The Minerva-Australis telescope array is a facility dedicated to the follow-up, confirmation, characterization, and mass measurement of planets orbiting bright stars discovered by the TransitingExpand
Post-main-sequence planetary system evolution
  • D. Veras
  • Physics, Medicine
  • Royal Society Open Science
  • 2016
The diverse dynamical processes which affect planets, asteroids, comets and pebbles as their parent stars evolve into giant branch, white dwarf and neutron stars are reviewed. Expand
Youth plus experience: the discovery of 51 Pegasi b
In 1995, Michel Mayor and Didier Queloz announced they discovered 51 Pegasi b, the first planet ever found around a star other than the Sun. This discovery turned out to be a milestone of recentExpand
Possibility of Detection of Exomoons with Inclined Orbits Orbiting Pulsar Planets Using the Time-of-Arrival Analysis
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 anExpand
Lab life: Don't bristle at blunders
In a July 1991 Nature paper, astronomers Andrew Lyne, Matthew Bailes and S. L. Shemar made an electrifying announcement: the discovery of the first planet outside our Solar System. To everyone’sExpand
Origin of apparent period variations in eclipsing post-common-envelope binaries
Apparent period variations detected in several eclipsing, close-compact binaries are frequently interpreted as being caused by circumbinary giant planets. This interpretation raises the question ofExpand
Discovery of pulsar planets
Abstract In this paper I recount the events which have led to the discovery of the first planets beyond the Solar System. The two planets circling an old neutron star, the 6.2 ms pulsar PSR B1257+12,Expand


A planetary system around the millisecond pulsar PSR1257 + 12
MILLISECOND radio pulsars, which are old (∼109yr), rapidly rotating neutron stars believed to be spun up by accretion of matter from their stellar companions, are usually found in binary systems withExpand
A planet orbiting the neutron star PSR1829–10
CONVENTIONAL optical techniques for detecting companions to stars have been unable to confirm the existence of other planetary systems. This is because of the small angular separation (less than anExpand