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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Proceedings ArticleDOI
Modeling Phase-resolved Observations of the Surfaces of Magnetic Neutron Stars
Wynn C. G. Ho,Kaya Mori +1 more
TL;DR: In this article, the shape and strength of the rotational variations in the total brightness and spectrum of two of the most observed neutron stars, RX J1856.5−3754 and 1E 1207.4−5209, were analyzed.
Journal ArticleDOI
Enhanced x-ray emission coinciding with giant radio pulses from the Crab Pulsar
Teruaki Enoto,Toshio Terasawa,Shota Kisaka,Shota Kisaka,Chin-Ping Hu,Chin-Ping Hu,Sebastien Guillot,Natalia Lewandowska,Christian Malacaria,Christian Malacaria,Paul S. Ray,Wynn C. G. Ho,Wynn C. G. Ho,Alice K. Harding,Alice K. Harding,Takashi Okajima,Zaven Arzoumanian,Keith C. Gendreau,Zorawar Wadiasingh,Zorawar Wadiasingh,Craig B. Markwardt,Yang Soong,Steve Kenyon,Slavko Bogdanov,Walid A. Majid,Tolga Guver,Gaurava K. Jaisawal,R. S. Foster,Yasuhiro Murata,Yasuhiro Murata,Hiroshi Takeuchi,Hiroshi Takeuchi,Kazuhiro Takefuji,Kazuhiro Takefuji,Mamoru Sekido,Yoshinori Yonekura,Hiroaki Misawa,Fuminori Tsuchiya,Takahiko Aoki,Munetoshi Tokumaru,Mareki Honma,Mareki Honma,Osamu Kameya,Tomoaki Oyama,Katsuaki Asano,Shinpei Shibata,Shuta J. Tanaka +46 more
TL;DR: In this article, the authors observed the Crab Pulsar simultaneously at x-ray and radio wavelengths, finding enhancement of the xray emission by 3.8 ± 0.7% (a 5.4σ detection).
Journal ArticleDOI
Mass/Radius Constraints on the Quiescent Neutron Star in M13 Using Hydrogen and Helium Atmospheres
Andrei Catuneanu,Andrei Catuneanu,Craig O. Heinke,Gregory R. Sivakoff,Wynn C. G. Ho,Mathieu Servillat +5 more
TL;DR: In this paper, the mass and radius of a quiescent neutron star in low-mass X-ray binaries were obtained by fitting the spectrum of the NS in quiescence.
Journal ArticleDOI
Magnetic Hydrogen Atmosphere Models and the Neutron Star RX J1856.5-3754
Wynn C. G. Ho,Wynn C. G. Ho,David L. Kaplan,Philip Chang,Philip Chang,Matthew van Adelsberg,Alexander Y. Potekhin +6 more
TL;DR: In this article, a model of a thin, magnetic, partially ionized hydrogen atmosphere on top of a condensed surface can fit the entire spectrum, from X-rays to optical, of RX J1856.5-3754, within the uncertainties.