Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/36514
Title: Ginga and ROSAT observations of AO Psc and V1223 Sgr
Authors: Taylor, P.
Beardmore, A. P.
Norton, A. J.
Osborne, Julian Paul
Watson, M. G.
First Published: 1-Aug-1997
Publisher: Blackwell Science Ltd
Citation: Monthly Notices Of The Royal Astronomical Society, 1997, 289 (2), pp. 349-354 (6)
Abstract: We present results from X-ray observations of the intermediate polars AO Psc and V1223 Sgr, taken with the ROSAT HRI and the Ginga LAC. Both sources show sinusoidal modulation at the white dwarf spin period in all energy bands, possibly with the exception of the highest. The depths of these modulations increase at lower energy, but the rates at which they do so are not consistent with single column densities of absorbing material. Neither source shows any significant pulse at the beat period, which argues for a predominantly disc-fed accretion model in each case. The AO Psc observations show a modulation at the orbital period, which in the ROSAT data may indicate an extended absorbing structure, with a dip at orbital phase ∼0.5– 0.8 superimposed. The V1223 Sgr ROSAT data show short dips which occur intermittently at around orbital phase 0.8. These dips vary in duration and phase of commencement and suggest that the system inclination angle is just sufficient for our line of sight to graze the upper extent of the material thrown out of the disc plane.
DOI Link: 10.1093/mnras/289.2.349
ISSN: 0035-8711
eISSN: 1365-2966
Links: http://mnras.oxfordjournals.org/content/289/2/349.short
http://hdl.handle.net/2381/36514
Version: Publisher Version
Status: Peer-reviewed
Type: Journal Article
Rights: Copyright © 1997 the authors. Monthly Notices of the Royal Astronomical Society © 1997 RAS. All rights reserved. Deposited with reference to the publisher’s archiving policy available on the SHERPA/RoMEO website.
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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