M
M. H. van Kerkwijk
Researcher at University of Toronto
Publications - 192
Citations - 13951
M. H. van Kerkwijk is an academic researcher from University of Toronto. The author has contributed to research in topics: Neutron star & Pulsar. The author has an hindex of 52, co-authored 183 publications receiving 11762 citations. Previous affiliations of M. H. van Kerkwijk include Max Planck Society & California Institute of Technology.
Papers
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Journal ArticleDOI
Optical and Infrared Observations of SGR 1806-20
Shrinivas R. Kulkarni,Keith Matthews,G. Neugebauer,I. N. Reid,M. H. van Kerkwijk,Gautam Vasisht +5 more
TL;DR: In this paper, the authors detect three objects in the vicinity of the radio core and infer that the star closest to the core is a supergiant, which is consistent with the high extinction (A_v ≥ 30 mag) that has been inferred for AX 1805.
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The Temperature and Cooling Age of the White Dwarf Companion to the Millisecond Pulsar PSR B1855+09.
TL;DR: In this article, the authors detect the binary millisecond pulsar PSR B1855+09 and detect its white dwarf companion and measure mF555W=25.90+/-0.12 and mF814W=24.19+/- 0.11 (Vega system).
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A 1500-MHz survey for pulsars near the Galactic Centre
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Time-resolved optical spectroscopy of the pulsating DA white dwarf HS 0507+0434B : New constraints on mode identification and pulsation properties
TL;DR: In this article, a detailed analysis of time-resolved optical spectra of the ZZ Ceti white dwarf, HS 0507+0434B, is presented.
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The Temperature and Cooling Age of the White-Dwarf Companion to the Millisecond Pulsar PSR B1855+09
TL;DR: On Keck and Hubble Space Telescope observations of the binary millisecond pulsar PSR B1855+09, it is inferred that helium white dwarfs form with thick hydrogen layers, with mass greater, similar3x10-3 M middle dot in circle, which leads to significant additional heating.