Search Results - "Higginbottom, N"

Thermal Disk Winds in X-Ray Binaries: Realistic Heating and Cooling Rates Give Rise to Slow, but Massive, Outflows by Higginbottom, N., Proga, D., Knigge, C., Long, K. S.

“…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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The impact of accretion disc winds on the optical spectra of cataclysmic variables by Matthews, J H, Knigge, C, Long, K S, Sim, S A, Higginbottom, N

“…Many high-state non-magnetic cataclysmic variables (CVs) exhibit blueshifted absorption or P-Cygni profiles associated with ultraviolet (UV) resonance lines…”
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Testing quasar unification: radiative transfer in clumpy winds by Matthews, J. H., Knigge, C., Long, K. S., Sim, S. A., Higginbottom, N., Mangham, S. W.

“…Various unification schemes interpret the complex phenomenology of quasars and luminous active galactic nuclei (AGN) in terms of a simple picture involving a…”
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A transient ultraviolet outflow in the short-period X-ray binary UW CrB by Fijma, S, Castro Segura, N, Degenaar, N, Knigge, C, Higginbottom, N, Hernández Santisteban, J V, Maccarone, T J

“…ABSTRACT Accreting low-mass X-ray binaries (LMXBs) are capable of launching powerful outflows such as accretion disc winds. In disc winds, vast amounts of…”
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A simple disc wind model for broad absorption line quasars by Higginbottom, N., Knigge, C., Long, K. S., Sim, S. A., Matthews, J. H.

“…Approximately 20 per cent of quasi-stellar objects (QSOs) exhibit broad, blue-shifted absorption lines in their ultraviolet spectra. Such features provide…”
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Do reverberation mapping analyses provide an accurate picture of the broad-line region? by Mangham, S W, Knigge, C, Williams, P, Horne, Keith, Pancoast, A, Matthews, J H, Long, K S, Sim, S A, Higginbottom, N

“…Abstract Reverberation mapping (RM) is a powerful approach for determining the nature of the broad-line region (BLR) in active galactic nuclei. However,…”
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The reverberation signatures of rotating disc winds in active galactic nuclei by Mangham, S. W., Knigge, C., Matthews, J. H., Long, K. S., Sim, S. A., Higginbottom, N.

“…Abstract The broad emission lines (BELs) in active galactic nuclei (AGNs) respond to ionizing continuum variations. The time and velocity dependence of their…”
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An efficient hybrid MAC protocol for high-speed LANs by Senior, J.M., Higginbottom, G.N.

“…This paper investigates the effects of asymmetric traffic load distributions and increasing data transmission rates on the operation of two types of hybrid…”
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A transient ultraviolet outflow in the short-period X-ray binary UW CrB by Fijma, S, Segura, N. Castro, Degenaar, N, Knigge, C, Higginbottom, N, Santisteban, J. V. Hernández, Maccarone, T. J

“…Accreting low mass X-ray binaries (LMXBs) are capable of launching powerful outflows such as accretion disc winds. In disc winds, vast amounts of material can…”
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Do Reverberation Mapping Analyses Provide an Accurate Picture of the Broad Line Region? by Mangham, S. W, Knigge, C, Williams, P, Horne, Keith, Pancoast, A, Matthews, J. H, Long, K. S, Sim, S. A, Higginbottom, N

“…Reverberation mapping (RM) is a powerful approach for determining the nature of the broad-line region (BLR) in active galactic nuclei. However, inferring…”
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The reverberation signatures of rotating disc winds in active galactic nuclei by Mangham, S. W, Knigge, C, Matthews, J. H, Long, K. S, Sim, S. A, Higginbottom, N

“…The broad emission lines (BELs) in active galactic nuclei (AGN) respond to ionizing continuum variations. The time and velocity dependence of their response…”
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A Simple Disk Wind Model for Broad Absorption Line Quasars by Higginbottom, N, Knigge, C, Long, K. S, Sim, S. A, Matthews, J. H

“…Approximately 20% of quasi-stellar objects (QSOs) exhibit broad, blue-shifted absorption lines in their ultraviolet spectra. Such features provide clear…”
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A spectral survey of the Star Forming Core of the Orion Nebula from 455 -- 507 GHz by White, Glenn J, Araki, M, Greaves, J. S, Ohishi, M, Higginbottom, N. S

“…Astron.Astrophys. 407 (2003) 589-608 The results of a submillimetre wavelength spectral line survey between 455.1 -- 507.4 GHz of the Orion-KL hot cloud core…”
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