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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.

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Spin period change and the magnetic fields of neutron stars in Be X-ray binaries in the SMC

TL;DR: In this article, the long term average spin period, rate of change of spin period and X-ray luminosity during outbursts for 42 Be Xray binary systems in the Small Mag- ellanic Cloud were reported.
Journal ArticleDOI

NSMAXG: A new magnetic neutron star spectral model in XSPEC

Wynn C. G. Ho
TL;DR: In this article, a magnetic atmosphere model of neutron stars is presented, which allows for more robust extractions of neutron star parameters from X-ray observations, and the NSMAXG implementation of these models in XSPEC is described.
Journal ArticleDOI

Signatures of photon-axion conversion in the thermal spectra and polarization of neutron stars

TL;DR: In this article, a detailed calculation aimed at quantifying the signatures of photon-axion conversion in the spectra, light curves, and polarization of neutron stars (NSs) is performed, taking into account the energy and angle dependence of the conversion probability and the surface thermal emission from NSs.
Posted Content

Constraints from LIGO O3 data on gravitational-wave emission due to r-modes in the glitching pulsar PSR J0537-6910

Richard J. Abbott, +1594 more
TL;DR: In this article, a search for continuous gravitational-wave emission due to r-modes in the pulsar PSR J0537-6910 using data from the LIGO-Virgo Collaboration observing run O3 was presented.