Search Results - "Higginbottom, Nick"
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CORONAE AND WINDS FROM IRRADIATED DISKS IN X-RAY BINARIES
Published in The Astrophysical journal (01-07-2015)“…ABSTRACT X-ray and UV line emission in X-ray binaries (XRBs) can be accounted for by a hot corona. Such a corona forms through irradiation of the outer disk by…”
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Thermally driven winds in ultraluminous X-ray sources
Published in Monthly notices of the Royal Astronomical Society (01-01-2022)“…ABSTRACT The presence of radiatively driven outflows is well established in ultraluminous X-ray sources (ULXs). These outflows are optically thick and can…”
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LINE-DRIVEN DISK WINDS IN ACTIVE GALACTIC NUCLEI: THE CRITICAL IMPORTANCE OF IONIZATION AND RADIATIVE TRANSFER
Published in The Astrophysical journal (01-07-2014)“…Accretion disk winds are thought to produce many of the characteristic features seen in the spectra of active galactic nuclei (AGNs) and quasi-stellar objects…”
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Stratified disc wind models for the AGN broad-line region: ultraviolet, optical, and X-ray properties
Published in Monthly notices of the Royal Astronomical Society (11-03-2020)“…ABSTRACT The origin, geometry, and kinematics of the broad-line region (BLR) gas in quasars and active galactic nuclei (AGN) are uncertain. We demonstrate that…”
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State-of-the-art simulations of line-driven accretion disc winds: realistic radiation hydrodynamics leads to weaker outflows
Published in Monthly notices of the Royal Astronomical Society (01-01-2024)“…ABSTRACT Disc winds are a common feature in accreting astrophysical systems on all scales. In active galactic nuclei (AGNs) and accreting white dwarfs (AWDs),…”
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Optical line spectra of tidal disruption events from reprocessing in optically thick outflows
Published in Monthly notices of the Royal Astronomical Society (01-03-2022)“…ABSTRACT A significant number of tidal disruption events (TDEs) radiate primarily at optical and ultraviolet (UV) wavelengths, with only weak soft X-ray…”
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Thermal and radiation driving can produce observable disc winds in hard-state X-ray binaries
Published in Monthly notices of the Royal Astronomical Society (11-03-2020)“…ABSTRACT X-ray signatures of outflowing gas have been detected in several accreting black hole binaries, always in the soft state. A key question raised by…”
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The luminosity dependence of thermally driven disc winds in low-mass X-ray binaries
Published in Monthly notices of the Royal Astronomical Society (21-04-2019)“…Abstract We have carried out radiation-hydrodynamic simulations of thermally driven accretion disc winds in low-mass X-ray binaries. Our main goal is to study…”
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Accretion disc winds in tidal disruption events: ultraviolet spectral lines as orientation indicators
Published in Monthly notices of the Royal Astronomical Society (01-06-2020)“…ABSTRACT Some tidal disruption events (TDEs) exhibit blueshifted broad absorption lines (BALs) in their rest-frame ultraviolet (UV) spectra, while others…”
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State-of-the-art simulations of line-driven accretion disc winds: realistic radiation-hydrodynamics leads to weaker outflows
Published 10-12-2023“…Disc winds are a common feature in accreting astrophysical systems on all scales. In active galactic nuclei (AGN) and accreting white dwarfs (AWDs),…”
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12
Thermally driven winds in ULXs
Published 15-10-2021“…The presence of radiatively driven outflows is well established in ultraluminous X-ray sources (ULXs). These outflows are optically thick and can reprocess a…”
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SIROCCO: A Publicly Available Monte Carlo Ionization and Radiative Transfer Code for Astrophysical Outflows
Published 25-10-2024“…Outflows are critical components of many astrophysical systems, including accreting compact binaries and active galactic nuclei (AGN). These outflows can…”
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14
Coronae and Winds from Irradiated Disks in X-ray binaries
Published 22-05-2015“…ApJ, 807, 107, 2015 X-ray and UV line emission in X-ray binaries can be accounted for by a hot corona. Such a corona forms through irradiation of the outer…”
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15
Optical line spectra of tidal disruption events from reprocessing in optically thick outflows
Published 05-01-2022“…A significant number of tidal disruption events (TDEs) radiate primarily at optical and ultraviolet (UV) wavelengths, with only weak soft X-ray components. One…”
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Accretion Disc Winds in Tidal Disruption Events: Ultraviolet Spectral Lines as Orientation Indicators
Published 16-04-2020“…Some tidal disruption events (TDEs) exhibit blueshifted broad absorption lines (BALs) in their rest-frame ultraviolet (UV) spectra, while others display broad…”
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17
The luminosity dependence of thermally-driven disc winds in low-mass X-ray binaries
Published 28-01-2019“…We have carried out radiation-hydrodynamic simulations of thermally-driven accretion disc winds in low-mass X-ray binaries. Our main goal is to study the…”
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Thermal Disk Winds in X-ray Binaries: Realistic Heating and Cooling Rates Give Rise to Slow, but Massive Outflows
Published 28-12-2016“…A number of X-ray binaries exhibit clear evidence for the presence of disk winds in the high/soft state. A promising driving mechanism for these outflows is…”
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Radiation-hydrodynamic simulations of thermally-driven disc winds in X-ray binaries: A direct comparison to GRO J1655-40
Published 13-06-2018“…Essentially all low-mass X-ray binaries (LMXBs) in the soft state appear to drive powerful equatorial disc winds. A simple mechanism for driving such outflows…”
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20
Thermal and radiation driving can produce observable disk winds in hard-state X-ray binaries
Published 27-01-2020“…X-ray signatures of outflowing gas have been detected in several accreting black-hole binaries, always in the soft state. A key question raised by these…”
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