Search Results - "Home, Keith"

Photoionized Hβ emission in NGC 5548 : t breathes by CACKETT, Edward M, HOME, Keith

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Spiral structure in the accretion disc of the binary IP Pegasi by Steeghs, D, Harlaftis, E T, Horne, Keith

“…We have found the first convincing evidence for spiral structure in the accretion disk of a close binary. The eclipsing dwarf nova binary IP Peg, observed…”
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A survey for planetary transits in the field of NGC 7789 by Bramich, D. M., Horne, Keith, Bond, I. A., Street, R. A., Cameron, A. Collier, Hood, B., Cooke, J., James, D., Lister, T. A., Mitchell, D., Pearson, K., Penny, A., Quirrenbach, A., Safizadeh, N., Tsapras, Y.

“…We present results from 30 nights of observations of the open cluster NGC 7789 with the Wide Field Camera on the Isaac Newton Telescope, La Palma. From ∼900…”
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SuperWASP-North extrasolar planet candidates : candidates from fields 17h < RA < 18h by LISTER, T. A, WEST, R. G, EVANS, A, FITZSIMMONS, A, HASWELL, C. A, HETTIER, C, HODGKIN, S. T, HOME, Keith, IRWIN, J, KEENAN, F. P, NORTON, A. J, OSBORNE, J, WILSON, D. M, POLLACCO, D. L, RYANS, R, SKILLEN, I, WHEATLEY, P. J, BARNES, J. R, COLLIER CAMERON, A, CLARKSON, W. I, STREET, R. A, ENOCH, B, PARLEY, N. R, CHRISTIAN, D. J, KANE, S. R

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Results from the Wide Angle Search for Planets Prototype (WASP0) – II. Stellar variability in the Pegasus field by Kane, Stephen R., Lister, T. A., Collier Cameron, Andrew, Horne, Keith, James, David, Pollacco, Don L., Street, Rachel A., Tsapras, Yiannis

“…Recent wide field photometric surveys, which target a specific field for long durations, are ideal for studying both long- and short-period stellar…”
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Results from the Wide Angle Search for Planets Prototype (WASP0) — III. Planet hunting in the Draco field by Kane, Stephen R., Collier Cameron, Andrew, Horne, Keith, James, David, Lister, T. A., Pollacco, Don L., Street, Rachel A., Tsapras, Yiannis

“…The Wide Angle Search for Planets Prototype (WASP0) is a wide-field instrument used to search for extra-solar planets via the transit method. Here we present…”
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The Millennium Galaxy Catalogue: star counts and the structure of the Galactic stellar halo by Lemon, D. J., Wyse, Rosemary F. G., Liske, J., Driver, S. P., Horne, Keith

“…We derive a star catalogue generated from the images taken as part of the ∼37.5 deg2 Millennium Galaxy Catalogue. These data, alone and together with colours…”
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Multicolour eclipse studies of UU Aquarii — II. The accretion disc by Baptista, R., Steiner, J. E., Home, Keith

“…Maximum-entropy eclipse mapping techniques are used to obtain maps of the surface brightness distribution of the UU Aqr accretion disc in its high (V ≃ 13.5…”
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Erratum: Spiral structure in the accretion disc of the binary IP Pegasi by Steeghs, D., Harlaftis, E. T., Home, Keith

“…The paper ‘Spiral structure in the accretion disc of the binary IP Pegasi’ was published in Mon. Not. R. Astron. Soc. 290, L28–L32 (1997). Figs 1 and 2 of the…”
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Mapping the accretion region in AM Her Systems: ST LMi by Cropper, Mark, Horne, Keith

“…We have used the maximum entropy method to map the spatial extent of the X-ray and optical emission in the AM Her system ST LMi. The emission region is…”
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The spin period of the intermediate polar RX J0558+53 by Allan, Alasdair, Home, Keith, Hellier, Coel, Mukai, K., Barwig, H., Bennie, P.J., Hilditch, R.W.

“…The newly discovered intermediate polar RXJ0558+53 has been reported to have a spin period of 272 s. We find modulations at both 272 and 545 s, implying that…”
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White dwarf radii and boundary-layer constraints in three dwarf novae by WOOD, J. H, HORNE, K

“…The structure of the boundary layer between the accretion disc and white dwarf in three quiescent dwarf novae is explored with high signal-to-noise eclipse…”
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HST observations of IP Pegasi in quiescence: the pre-eclipse spectrum by Hoard, D. W., Baptista, Raymundo, Eracleous, Michael, Home, Keith, Misselt, K. A., Shatter, Allen W., Szkody, Paula, Wood, Janet H.

“…We present time-resolved HST ultraviolet (UV) spectroscopy and ground-based optical photometry of the dwarf nova IP Pegasi in a quiescent state. The…”
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