Search Results - "Salvesen, Greg"
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1
Shock Speed, Cosmic Ray Pressure, and Gas Temperature in the Cygnus Loop
Published in The Astrophysical journal (01-09-2009)“…Upper limits on the shock speeds in supernova remnants can be combined with post-shock temperatures to obtain upper limits on the ratio of cosmic ray to gas…”
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Journal Article -
2
An Electron-scattering Time Delay in Black Hole Accretion Disks
Published in Astrophysical journal. Letters (01-11-2022)“…Abstract Universal to black hole X-ray binaries, the high-frequency soft lag gets longer during the hard-to-intermediate state transition, evolving from ≲1 to…”
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Journal Article -
3
Origin of spin–orbit misalignments: the microblazar V4641 Sgr
Published in Monthly notices of the Royal Astronomical Society (01-06-2020)“…ABSTRACT Of the known microquasars, V4641 Sgr boasts the most severe lower limit (>52°) on the misalignment angle between the relativistic jet axis and the…”
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Journal Article -
4
A physical model for state transitions in black hole X-ray binaries
Published in Monthly notices of the Royal Astronomical Society (01-02-2014)“…We present an accretion cycle which can explain state transitions and other observed phenomena in black hole X-ray binaries. This model is based on the process…”
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Journal Article -
5
Black hole spin in X-ray binaries: giving uncertainties an f
Published in Monthly notices of the Royal Astronomical Society (01-01-2021)“…ABSTRACT The two established techniques for measuring black hole spin in X-ray binaries often yield conflicting results, which must be resolved before either…”
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Journal Article -
6
Accretion disc dynamo activity in local simulations spanning weak-to-strong net vertical magnetic flux regimes
Published in Monthly notices of the Royal Astronomical Society (21-03-2016)“…Strongly magnetized accretion discs around black holes have attractive features that may explain enigmatic aspects of X-ray binary behaviour. The structure and…”
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Journal Article -
7
Strongly magnetized accretion discs require poloidal flux
Published in Monthly notices of the Royal Astronomical Society (21-08-2016)“…Motivated by indirect observational evidence for strongly magnetized accretion discs around black holes, and the novel theoretical properties of such…”
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Journal Article -
8
Convective quenching of field reversals in accretion disc dynamos
Published in Monthly notices of the Royal Astronomical Society (01-06-2017)Get full text
Journal Article -
9
Spectral hardening as a viable alternative to disc truncation in black hole state transitions
Published in Monthly notices of the Royal Astronomical Society (01-06-2013)“…Constraining the accretion flow geometry of black hole binaries in outburst is complicated by the inability of simplified multicolour disc models to…”
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Journal Article -
10
An Electron-Scattering Time Delay in Black Hole Accretion Disks
Published 28-09-2022“…Universal to black hole X-ray binaries, the high-frequency soft lag gets longer during the hard-to-intermediate state transition, evolving from…”
Get full text
Journal Article -
11
Quantifying energetics and dissipation in magnetohydrodynamic turbulence
Published in Monthly notices of the Royal Astronomical Society (21-02-2014)“…We perform a suite of two- and three-dimensional magnetohydrodynamic (MHD) simulations with the athena code of the non-driven Kelvin–Helmholtz instability in…”
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Journal Article -
12
Six-Day Footraces in the Post-Pedestrianism Era
Published 14-01-2019“…In a six-day footrace, competitors accumulate as much distance as possible on foot over 144 consecutive hours by circumambulating a loop course. Now an obscure…”
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Journal Article -
13
SHOCK SPEED, COSMIC RAY PRESSURE, AND GAS TEMPERATURE IN THE CYGNUS LOOP
Published in The Astrophysical journal (01-09-2009)“…Upper limits on the shock speeds in supernova remnants can be combined with post-shock temperatures to obtain upper limits on the ratio of cosmic ray to gas…”
Get full text
Journal Article -
14
Origin of Spin-Orbit Misalignments: The Microblazar V4641 Sgr
Published 25-06-2020“…Of the known microquasars, V4641 Sgr boasts the most severe lower limit (> 52{\deg}) on the misalignment angle between the relativistic jet axis and the binary…”
Get full text
Journal Article -
15
Black Hole Spin in X-ray Binaries: Giving Uncertainties an $f
Published 22-10-2020“…The two established techniques for measuring black hole spin in X-ray binaries often yield conflicting results, which must be resolved before either method may…”
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Journal Article -
16
Rethinking Black Hole Accretion Discs
Published 01-01-2016“…Accretion discs are staples of astrophysics. Tapping into the gravitational potential energy of the accreting material, these discs are highly efficient…”
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Dissertation -
17
A physical model for state transitions in black hole X-ray binaries
Published 12-11-2013“…We present an accretion cycle which can explain state transitions and other observed phenomena in black hole X-ray binaries. This model is based on the process…”
Get full text
Journal Article -
18
Convective Quenching of Field Reversals in Accretion Disc Dynamos
Published 27-01-2017“…Vertically stratified shearing box simulations of magnetorotational turbulence commonly exhibit a so-called butterfly diagram of quasi-periodic azimuthal field…”
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Journal Article -
19
Strongly magnetized accretion discs require poloidal flux
Published 18-05-2016“…Motivated by indirect observational evidence for strongly magnetized accretion discs around black holes, and the novel theoretical properties of such…”
Get full text
Journal Article -
20
Accretion disc dynamo activity in local simulations spanning weak-to-strong net vertical magnetic flux regimes
Published 12-01-2016“…Strongly magnetized accretion discs around black holes have attractive features that may explain enigmatic aspects of X-ray binary behaviour. The structure and…”
Get full text
Journal Article