T
Tom Marsh
Researcher at University of Warwick
Publications - 433
Citations - 20173
Tom Marsh is an academic researcher from University of Warwick. The author has contributed to research in topics: White dwarf & Stars. The author has an hindex of 63, co-authored 401 publications receiving 18418 citations. Previous affiliations of Tom Marsh include Space Telescope Science Institute & University of Oxford.
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Journal ArticleDOI
A massive pulsar in a compact relativistic binary
John Antoniadis,Paulo C. C. Freire,Norbert Wex,Thomas M. Tauris,Ryan S. Lynch,Marten H. van Kerkwijk,Michael Kramer,Michael Kramer,C. G. Bassa,V. S. Dhillon,T. Driebe,Jason W. T. Hessels,Jason W. T. Hessels,Victoria M. Kaspi,V. I. Kondratiev,V. I. Kondratiev,Norbert Langer,Tom Marsh,Maura McLaughlin,Timothy T. Pennucci,Scott M. Ransom,Ingrid H. Stairs,Joeri van Leeuwen,Joeri van Leeuwen,Joris P. W. Verbiest,David G. Whelan +25 more
TL;DR: Pulsar J0348+0432 is only the second neutron star with a precisely determined mass of 2 M☉
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The origin of subdwarf B stars – I. The formation channels
TL;DR: In this paper, a detailed investigation of the three main binary evolution channels that can lead to the formation of sdB stars: the common-envelope (CE) ejection channel, the stable Roche lobe overflow (RLOF) channel, and the double helium white dwarfs (WDs) merger channel is presented.
Journal ArticleDOI
The origin of subdwarf B stars – II
TL;DR: In this article, a detailed binary population synthesis (BPS) study of the formation of subdwarf B (sdB) stars and related objects (sdO, sdOB stars) using the latest version of the BPS code developed by Han and co-workers was carried out.
Journal ArticleDOI
The Origin of Subdwarf B Star (I): the Formation Channels
TL;DR: In this article, the authors investigated the three main binary evolution channels that can lead to the formation of sdB stars: the common envelope (CE) ejection channel, the stable Roche lobe overflow (RLOF) channel and the double helium white dwarfs (WDs) merger channel.
Journal ArticleDOI
The origin of sdB stars (II)
TL;DR: Han et al. as discussed by the authors carried out a detailed binary populations synthesis (BPS) study of the formation of subdwarf B (sdB) stars and related objects using the latest version of the BPS code developed by Han et al (1994, 1995a, 1995b, 1998, 2001).