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
X-ray and Radio Variabilities of PSR J2032+4127 near Periastron
Chi-Yung Ng,Wynn C. G. Ho,Wynn C. G. Ho,Eric V. Gotthelf,Jules P. Halpern,M. J. Coe,Benjamin Stappers,Andrew Lyne,K. S. Wood,Matthew Kerr +9 more
TL;DR: In this paper, the gamma-ray and radio monitoring observations of the Gamma-ray binary PSR J2032+4127/MT91 213 during its periastron passage in late 2017 were presented.
Journal ArticleDOI
Constraints on neutron star superfluidity from the cooling neutron star in Cassiopeia A using all Chandra ACIS-S observations
TL;DR: In this paper , a joint spectral analysis using all Chandra data was performed to constrain the mass of the Cassiopeia A NS at 1 . 55 ± 0 . 25 ǫ (cid:12) , and its radius at 13 . 5 ± 1 . 5 km.
Journal Article
Supernovae and Their Consequences: Studies with the Generation-X Mission
Patrick Slane,Stephen P. Reynolds,Alicia M. Soderberg,John P. Hughes,Jacco Vink,Wynn C. G. Ho,Daniel J. Patnaude,David Pooley,Robert Petre,Sangwook Park,Carles Badenes,Randall K. Smith,Roger Brissenden +12 more
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.
Book ChapterDOI
Modeling Spectral Features from Isolated Neutron Stars
TL;DR: In this article, the authors studied several effects that influence the strength of the proton cyclotron and atomic features in the thermal spectra of magnetic neutron stars, showing that magnetic field variations over the neutron star surface leads to broadening of features.