Search Results - "Laycock, S. G."
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A multi‐observatory database of X‐ray pulsars in the Magellanic Clouds
Published in Astronomische Nachrichten (01-03-2017)“…Using hundreds of XMM‐Newton and Chandra archival observations and nearly a thousand RXTE observations, we have generated a comprehensive library of the known…”
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2
A Comprehensive Library of X-Ray Pulsars in the Small Magellanic Cloud: Time Evolution of Their Luminosities and Spin Periods
Published in The Astrophysical journal (20-04-2017)“…We have collected and analyzed the complete archive of XMM-Newton (116), Chandra (151), and RXTE (952) observations of the Small Magellanic Cloud (SMC),…”
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3
Not an Oxymoron: Some X-Ray Binary Pulsars with Enormous Spin-Up Rates Reveal Weak Magnetic Fields
Published in Monthly notices of the Royal Astronomical Society (01-08-2018)“…Three high-mass X-ray binaries have been discovered recently exhibiting enormous spin-up rates. Conventional accretion theory predicts extremely high-surface…”
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4
Retrograde accretion discs in high-mass Be/X-ray binaries
Published in Monthly notices of the Royal Astronomical Society. Letters (01-09-2017)“…Abstract We have compiled a comprehensive library of all X-ray observations of Magellanic pulsars carried out by XMM–Newton, Chandra and RXTE in the period…”
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5
On the Geometry of the X-ray emission from pulsars a consistent inclination and beaming solution for the Be/X-ray pulsar SXP 1062
Published in Monthly notices of the Royal Astronomical Society (01-06-2020)“…ABSTRACT SXP 1062 is a long-period X-ray pulsar (XRP) with a Be optical companion located in the Small Magellanic Cloud. First discovered in 2010 from…”
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On the geometry of the X-ray emission from pulsars: the changing aspect of the Be/X-ray pulsar SXP348
Published in Monthly notices of the Royal Astronomical Society (01-07-2019)“…The X-ray source SXP348 is a high-mass X-ray binary system in the Small Magellanic Cloud. Since its 1998 discovery by BeppoSAX, this pulsar has exhibited a…”
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Disentangling the neighbouring pulsars SXP 15.3 and SXP 305
Published in Monthly notices of the Royal Astronomical Society (12-03-2022)“…ABSTRACT SXP 15.3 and SXP 305 are two Be X-ray binaries in the Small Magellanic Cloud that are spatially separated by ∼7 arcsec. The small separation between…”
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8
Multiwavelength observations of the Be/X-ray binary IGR J01217−7257 (=SXP 2.16) during outburst
Published in Monthly notices of the Royal Astronomical Society (01-04-2017)“…We present simultaneous, multiwavelength observations of the Small Magellanic Cloud Be/XRB IGR J01217-7257 (=SXP 2.16) during outbursts in 2014, 2015 and 2016…”
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9
Constraints on the number of X‐ray pulsars in IC 10 from a deep XMM‐Newton observation
Published in Astronomische Nachrichten (01-01-2019)“…We report the most sensitive search yet for X‐ray pulsars in the dwarf starburst galaxy IC 10, which is known to contain a population of young, high‐mass X‐ray…”
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10
Evolution of high‐mass X‐ray binaries in the small magellanic cloud
Published in Astronomische Nachrichten (01-01-2019)“…To understand the progenitor of rotation‐powered pulsars, we compare them with accreting High‐Mass X‐ray binary pulsars, (hereafter X‐ray pulsars), in the…”
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11
On the Theoretical Framework of Magnetized Outflows from Stellar-Mass Black Holes and Related Observations
Published in Monthly notices of the Royal Astronomical Society (21-09-2016)“…The spins of stellar-mass black holes (BHs) and the power outputs of their jets are measurable quantities. Unfortunately, the currently employed methods do not…”
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12
Optical studies of two Large Magellanic Cloud X-ray transients: RX J0544.1–7100 and RX J0520.5–6932
Published in Monthly notices of the Royal Astronomical Society (01-07-2001)“…We report observations that confirm the identities of the optical counterparts to the transient sources RX J0544.1–7100 and RX J0520.5–6932. The counterparts…”
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13
Not an Oxymoron: Some X-ray Binary Pulsars with Enormous Spinup Rates Reveal Weak Magnetic Fields
Published 15-05-2018“…Three high-mass X-ray binaries have been discovered recently exhibiting enormous spinup rates. Conventional accretion theory predicts extremely high surface…”
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14
A Striking Confluence Between Theory and Observations of High-Mass X-ray Binary Pulsars
Published 09-01-2018“…We analyse the most powerful X-ray outbursts from neutron stars in ten Magellanic high-mass X-ray binaries and three pulsating ultraluminous X-ray sources…”
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15
Observations of the unusual counterpart to the X-ray pulsar AX J0051−733
Published in Monthly notices of the Royal Astronomical Society (01-05-2002)“…Abstract We report optical and infrared (IR) observations of the ASCA X-ray pulsar system AX J0051−733. The relationship between the X-ray source and possible…”
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16
The Great Pretenders Among the ULX Class
Published 24-03-2017“…The recent discoveries of pulsed X-ray emission from three ultraluminous X-ray (ULX) sources have finally enabled us to recognize a subclass within the ULX…”
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17
A Comprehensive Library of X-ray Pulsars in the Small Magellanic Cloud: Time Evolution of their Luminosities and Spin Periods
Published 15-03-2017“…We have collected and analyzed the complete archive of {\itshape XMM-Newton\} (116), {\itshape Chandra\} (151), and {\itshape RXTE\} (952) observations of the…”
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Journal Article -
18
A multi-observatory database of X-ray pulsars in the Magellanic Clouds
Published 14-03-2017“…Using hundreds of XMM-Newton and Chandra archival observations and nearly a thousand RXTE observations, we have generated a comprehensive library of the known…”
Get full text
Journal Article -
19
On the Theoretical Framework of Magnetized Outflows from Stellar-Mass Black Holes and Related Observations
Published 21-06-2016“…The spins of stellar-mass black holes (BHs) and the power outputs of their jets are measurable quantities. Unfortunately, the currently employed methods do not…”
Get full text
Journal Article -
20
Multi-wavelength observations of the Be/X-ray binary IGR J01217-7257 (=SXP 2.16) during outburst
Published 02-12-2016“…We present simultaneous, multi-wavelength observations of the Small Magellanic Cloud Be/XRB IGR J01217-7257 (=SXP 2.16) during outbursts in 2014, 2015 and…”
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Journal Article