The relation between white dwarf mass and orbital period in wide binary radio pulsars
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This article is published in Monthly Notices of the Royal Astronomical Society.The article was published on 1995-04-01 and is currently open access. It has received 237 citations till now. The article focuses on the topics: Binary pulsar & White dwarf.read more
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Journal ArticleDOI
Relativistic Shapiro delay measurements of an extremely massive millisecond pulsar
H. T. Cromartie,Emmanuel Fonseca,Scott M. Ransom,Paul Demorest,Zaven Arzoumanian,Harsha Blumer,Paul R. Brook,Megan E. DeCesar,Timothy Dolch,Justin A. Ellis,Robert D. Ferdman,Elizabeth C. Ferrara,Elizabeth C. Ferrara,N. Garver-Daniels,Peter A. Gentile,M. L. Jones,Michael T. Lam,Duncan R. Lorimer,Ryan S. Lynch,Maura McLaughlin,Cherry Ng,Cherry Ng,David J. Nice,Timothy T. Pennucci,Renée Spiewak,Ingrid H. Stairs,Kevin Stovall,Joseph K. Swiggum,Weiwei Zhu +28 more
TL;DR: In this article, the authors measured the mass of the MSP J0740+6620 to be ${\mathbf{2.14} + 2.09} + 0.10% credibility interval.
Journal ArticleDOI
Relativistic Shapiro delay measurements of an extremely massive millisecond pulsar
H. Thankful Cromartie,Emmanuel Fonseca,Scott M. Ransom,Paul Demorest,Zaven Arzoumanian,Harsha Blumer,Paul R. Brook,Megan E. DeCesar,Timothy Dolch,Justin A. Ellis,Robert D. Ferdman,Elizabeth C. Ferrara,N. Garver-Daniels,P. A. Gentile,Megan L. Jones,Michael T. Lam,Duncan R. Lorimer,Ryan S. Lynch,Maura McLaughlin,Cherry Ng,David J. Nice,Timothy T. Pennucci,Renée Spiewak,Ingrid H. Stairs,Kevin Stovall,Joseph K. Swiggum,Weiwei Zhu +26 more
TL;DR: In this article, the relativistic Shapiro delay (Shapiro 1964) was used to estimate the masses of a pulsar binary system, and the mass of the binary system was found to be 2.14+0.10−0.18−1.
Journal ArticleDOI
Neutron Star Mass Measurements. I. Radio Pulsars
TL;DR: In this paper, the masses of radio pulsars and their companions are estimated from relativistic orbital effects, and significant constraints exist on the mass of 21 radio and five neutron star companions.
Journal ArticleDOI
Evolutionary Binary Sequences for Low- and Intermediate-Mass X-ray Binaries
TL;DR: In this paper, Tauris et al. present the results of a systematic study of the evolution of low and intermediate-mass X-ray binaries (LMXBs and IMXBs) using a standard Henyey-type stellar evolution code and a standard model for binary interactions.