W
Wynn C. G. Ho
Researcher at Haverford College
Publications - 234
Citations - 22680
Wynn C. G. Ho is an academic researcher from Haverford College. The author has contributed to research in topics: Neutron star & Pulsar. The author has an hindex of 57, co-authored 225 publications receiving 17033 citations. Previous affiliations of Wynn C. G. Ho include Massachusetts Institute of Technology & Stanford University.
Papers
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Journal ArticleDOI
Constraining the Neutron Star Mass--Radius Relation and Dense Matter Equation of State with NICER. III. Model Description and Verification of Parameter Estimation Codes
Slavko Bogdanov,Alexander J. Dittmann,Alexander J. Dittmann,Wynn C. G. Ho,Frederick K. Lamb,Simin Mahmoodifar,M. Coleman Miller,Sharon M. Morsink,Thomas E. Riley,Tod E. Strohmayer,Anna L. Watts,Devarshi Choudhury,Sebastien Guillot,Sebastien Guillot,Alice K. Harding,Paul S. Ray,Zorawar Wadiasingh,Zorawar Wadiasingh,Michael T. Wolff,Craig B. Markwardt,Zaven Arzoumanian,Keith C. Gendreau +21 more
TL;DR: In this article, the mass and radius estimates of rotation-powered millisecond pulsars were analyzed using the X-ray pulse profile models used to obtain information about the mass-radius relation of neutron stars and the equation of state of dense matter in their cores.
Journal ArticleDOI
Central compact objects and their magnetic fields
TL;DR: In this paper, X-ray timing and spectral measurements suggest CCOs have relatively weak surface magnetic fields (~ 1010 − 1011 G), and they argue that CCO are born with strong fields and we are only seeing a weak surface field that is transitory and evolving.
Journal ArticleDOI
A joint NICER and XMM-Newton view of the "Magnificent" thermally emitting X-ray Isolated Neutron Star RX J1605.3+3249
Christian Malacaria,Slavko Bogdanov,Wynn C. G. Ho,Teruaki Enoto,Paul S. Ray,Zaven Arzoumanian,Thoniel Cazeau,Keith C. Gendreau,Sebastien Guillot,Tolga Guver,Gaurava K. Jaisawal,Michael T. Wolff +11 more
TL;DR: In this article, the authors analyzed NICER and XMM-Newton observations of RX J1605.3+3249, in order to address its timing and spectral behavior, finding no significant pulsation with pulsed fraction higher than 1.3% (3σ) for periods above 150 ms.
Neutron Star Dense Matter Equation of State Constraints with NICER
Slavko Bogdanov,Zaven Arzoumanian,Deepto Chakrabarty,Sebastien Guillot,Alice K. Harding,Wynn C. G. Ho,Frederick K. Lamb,Simin Mahmoodifar,M. Coleman Miller,Sharon M. Morsink,Feryal Özel,Dimitrios Psaltis,Paul S. Ray,Thomas E. Riley,Tod E. Strohmayer,Anna L. Watts,Michael T. Wolff,Keith C. Gendreau +17 more
Journal ArticleDOI
Magnetars are super hot and super cool
TL;DR: In this article, the authors examined the role of magnetic field decay in the core of a neutron star and showed that extremely strong heating from field decay cannot produce the high observed surface temperatures nor delay the onset of neutron superfluidity.