Binary radio pulsars

267 citations recorded by the source corpus.

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

The evolution of binary fractions in globular clusters (2005, background): “…in detail the rare but important evolutionary channels that may pl y a crucial role in the formation of some of the most interestingtracers of dynamical interactions in dense clusters, such as ultracompact X-ray binaries, millisecond pulsars, and cataclysmicvariables (Ivanova & Rasio 2004a,b).”
Hypernuclear Physics for Neutron Stars (2008, background): “00035)M⊙ [2], the fastest rotating one is the pulsar PSR J1748-2446ad with 716 revolutions per second [3].”
Tidal deformability of neutron stars with realistic equations of state (2009, background): “5 M , which is conservatively low given recent neutron-star mass observations [24, 25, 26, 27, 28].”
Compact Object Modeling with the StarTrack Population Synthesis Code (2005, unknown): “Using X-ray studies of Galactic transient systems with NS accretors (e.g., Tavani & Arons 1997; Rutledge et al. 2001; Campana & Stella 2003; Jonker et al. 2004; Tomsick et al. 2004; Campana 2005), we adopt 1031 ergs s 1 as a lower limit for the hard X-ray luminosity, above 2 keV.”