THE FORMATION OF THE ECCENTRIC-ORBIT MILLISECOND PULSAR J1903+0327 AND THE ORIGIN OF SINGLE MILLISECOND PULSARS-Reference-Cited by-同舟云学术

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THE FORMATION OF THE ECCENTRIC-ORBIT MILLISECOND PULSAR J1903+0327 AND THE ORIGIN OF SINGLE MILLISECOND PULSARS

Published:2011-05-25 Issue:1 Volume:734 Page:55
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Portegies Zwart S.,van den Heuvel E. P. J.,van Leeuwen J.,Nelemans G.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/734/i=1/a=55/pdf

Reference65 articles.

1. A regularization of the three-body problem

2. A regularization of the three-body problem

3. A new class of radio pulsars

4. A Radio Pulsar/X-ray Binary Link

5. The Velocity Distribution of Isolated Radio Pulsars

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3. Impact of asymmetrical mass ejection from proto-white dwarfs on the properties of binary millisecond pulsars;Monthly Notices of the Royal Astronomical Society;2022-12-12

4. Forming hot subluminous stars from hierarchical triples – I. The role of an outer tertiary on formation channels;Monthly Notices of the Royal Astronomical Society;2022-10-07

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