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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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Multiwavelength observations of Be X-ray binary PSR J2032+4127/MT91 213 through periastron
Wynn C. G. Ho,M. J. Coe,Eric V. Gotthelf,Jules P. Halpern,Tyrel J. Johnson,Matthew Kerr,Chi-Yung Ng,Atsuo T. Okazaki,Paul S. Ray,Ben Stappers,Iain A. Steele +10 more
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On the 2018 outburst of the accreting millisecond X-ray pulsar Swift J1756.9-2508 as seen with NICER.
Peter Bult,Diego Altamirano,Zaven Arzoumanian,Deepto Chakrabarty,Keith C. Gendreau,Sebastien Guillot,Sebastien Guillot,Wynn C. G. Ho,Wynn C. G. Ho,Gaurava K. Jaisawal,Steven Lentine,Craig B. Markwardt,Son N. Ngo,J. Pope,Paul S. Ray,M. Saylor,Tod E. Strohmayer +16 more
TL;DR: In this paper, coherent timing analysis of the 182 Hz accreting millisecond X-ray pulsar Swift J1756 was performed with the Neutron Star Interior Composition Explorer (NICER).
Journal Article
全chandra x線観測衛星検出器によるcassiopeia aにおける中性子星の冷却の測定
K. G. Elshamouty,Craig O. Heinke,G. R. Sivakoff,Wynn C. G. Ho,P. S. Shternin,D. G. Yakovlev,Daniel J. Patnaude,Laurence P. David +7 more
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Atmospheres and Spectra of Strongly Magnetized Neutron Stars -- III. Partially Ionized Hydrogen Models
TL;DR: In this paper, the authors constructed partially ionized hydrogen atmosphere models for magnetized neutron stars in radiative equilibrium with surface fields B=10^12-5 \times 10^14 G and effective temperatures T_eff \sim a few K times 10^5-10^6 K.