Search Results - "van Kerkwijk, M H"
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The Delay Times of Type Ia Supernova
Published in The Astrophysical journal (01-09-2019)“…The delay time distribution of Type Ia supernovae (SNe Ia; the time-dependent rate of SNe resulting from a burst of star formation) has been measured using…”
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CHIME Discovery of a Binary Pulsar with a Massive Nondegenerate Companion
Published in The Astrophysical journal (01-01-2023)“…Abstract Of the more than 3000 radio pulsars currently known, only ∼300 are in binary systems, and only five of these consist of young pulsars with massive…”
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Isolated neutron stars: magnetic fields, distances,and spectra
Published in Astrophysics and space science (01-04-2007)“…We present timing measurements, astrometry, and high-resolution spectra of a number of nearby, thermally emitting, isolated neutron stars. We use these to…”
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Evidence for a Massive Neutron Star from a Radial-velocity Study of the Companion to the Black-widow Pulsar PSR B1957+20
Published in The Astrophysical journal (20-02-2011)“…The most massive neutron stars constrain the behavior of ultra-dense matter, with larger masses possible only for increasingly stiff equations of state. Here,…”
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Timing the Nearby Isolated Neutron Star RX J1856.5–3754
Published in The Astrophysical journal (01-02-2008)“…RX J1856.5-3754 is the X-ray brightest among the nearby isolated neutron stars. Its X-ray spectrum is thermal, and is reproduced remarkably well by a…”
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6
Merging white dwarfs and thermonuclear supernovae
Published in Philosophical transactions of the Royal Society of London. Series A: Mathematical, physical, and engineering sciences (13-06-2013)“…Thermonuclear supernovae result when interaction with a companion reignites nuclear fusion in a carbonoxygen white dwarf, causing a thermonuclear runaway, a…”
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A Dense Companion to the Short-period Millisecond Pulsar Binary PSR J0636+5128
Published in The Astrophysical journal (01-09-2018)“…PSR J0636+5128 is a millisecond pulsar in one of the most compact pulsar binaries known, with a 96 minute orbital period. The pulsar mass function suggests a…”
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Hubble Space Telescope Detection of the Millisecond Pulsar J2124−3358 and its Far-ultraviolet Bow Shock Nebula
Published in The Astrophysical journal (01-02-2017)“…We observed the nearby millisecond pulsar J2124-3358 with the Hubble Space Telescope in broad far-UV (FUV) and optical filters. The pulsar is detected in both…”
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Spectral Sequences of Type Ia Supernovae. I. Connecting Normal and Subluminous SNe Ia and the Presence of Unburned Carbon
Published in The Astrophysical journal (01-09-2017)“…Type Ia supernovae (SNe Ia) are generally agreed to arise from thermonuclear explosions of carbon-oxygen white dwarfs. The actual path to explosion, however,…”
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KOI 1224: A FOURTH BLOATED HOT WHITE DWARF COMPANION FOUND WITH KEPLER
Published in The Astrophysical journal (01-04-2012)“…We present an analysis and interpretation of the Kepler binary system KOI 1224. This is the fourth binary found with Kepler that consists of a thermally…”
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Measuring the mass of the black widow PSR J1555-2908
Published in Monthly notices of the Royal Astronomical Society (31-03-2022)“…ABSTRACT Accurate measurements of the masses of neutron stars are necessary to test binary evolution models, and to constrain the neutron star equation of…”
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12
An optical counterpart to the anomalous X-ray pulsar 4U0142+61
Published in Nature (London) (07-12-2000)“…The energy source of the anomalous X-ray pulsars (AXPs) is not understood, hence their designation as anomalous. Unlike binary X-ray pulsars, no companions are…”
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A Coherent Timing Solution for the Nearby Isolated Neutron Star RX J0720.4–3125
Published in The Astrophysical journal (20-07-2005)“…We present the results of a dedicated effort to measure the spin-down rate of the nearby isolated neutron star RX J0720.4-3125. Comparing arrival times of the…”
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Spectral Sequences of Type Ia Supernovae. II. Carbon as a Diagnostic Tool for Explosion Mechanisms
Published in The Astrophysical journal (01-02-2019)“…How an otherwise inert carbon-oxygen white dwarf can be made to explode as an SN Ia remains unknown. A promising test of theoretical models is to constrain the…”
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The Distance to the Isolated Neutron Star RX J0720.4–3125
Published in The Astrophysical journal (10-05-2007)“…We have used a set of dedicated astrometric data from the Hubble Space Telescope to measure the parallax and proper motion of the nearby neutron star RX…”
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The relativistic pulsar-white dwarf binary PSRJ1738+0333 - I. Mass determination and evolutionary history
Published in Monthly notices of the Royal Astronomical Society (01-07-2012)“…PSR J1738+0333 is one of the four millisecond pulsars known to be orbited by a white dwarf companion bright enough for optical spectroscopy. Of these, it has…”
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Constraining the Spin-down of the Nearby Isolated Neutron Star RX J0806.4–4123, and Implications for the Population of Nearby Neutron Stars
Published in The Astrophysical journal (01-11-2009)“…The nearby isolated neutron stars (INSs) are a group of seven relatively slowly rotating neutron stars that show thermal X-ray spectra, most with broad…”
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VLBA Measurement of the Transverse Velocity of the Magnetar XTE J1810–197
Published in The Astrophysical journal (20-06-2007)“…We have obtained observations of the magnetar XTE J1810-197 with the Very Long Baseline Array (VLBA) at two epochs separated by 106 days, at wavelengths of 6…”
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A Strong, Broad Absorption Feature in the X-Ray Spectrum of the Nearby Neutron Star RX J1605.3+3249
Published in The Astrophysical journal (10-06-2004)“…We present X-ray spectra taken with XMM-Newton of RX J1605.3+3249, the third brightest in the class of nearby thermally emitting neutron stars. In contrast to…”
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The Parallax and Proper Motion of RX J1856.5–3754 Revisited
Published in The Astrophysical journal (20-05-2002)Get full text
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