Issue |
A&A
Volume 440, Number 2, September III 2005
|
|
---|---|---|
Page(s) | 675 - 681 | |
Section | Stellar structure and evolution | |
DOI | https://doi.org/10.1051/0004-6361:20052950 | |
Published online | 01 September 2005 |
XMM-Newton observations of AM CVn binaries
1
Mullard Space Science Laboratory, University College London, Holmbury St Mary, Dorking, Surrey RH5 6NT, UK e-mail: gtbr@mssl.ucl.ac.uk
2
Observatory, PO Box 14, 00014 University of Helsinki, Finland
3
Department of Physics, University of Warwick, Coventry CV4 7AL, UK
4
Institue of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK
5
Department of Astrophysics, Radboud University of Nijmegen, PO Box 9010, 6500 Nijmegen, The Netherlands
6
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, MS-67, Cambridge, MA 02138, USA
Received:
28
February
2005
Accepted:
26
May
2005
We present the results of XMM-Newton observations of four AM CVn systems – AM CVn, CR Boo, HP Lib and GP Com. Their light
curves show very different characteristics. The X-ray light curves
show no coherent pulsations, suggesting the accreting white dwarfs
have relatively low magnetic field strengths. Their spectra were
best modelled using a multi-temperature emission model and a strong
UV component. We find that CR Boo and HP Lib have X-ray spectra
with abundances consistent with relatively low temperature CNO
processed material, while AM CVn and GP Com show an enhancement of
nitrogen. A large fraction of the accretion luminosity is emitted in
the UV. We determine accretion luminosities of
~ erg s-1 and
erg s-1 for AM CVn and GP Com respectively. Comparing the implied mass transfer
rates with that derived using model fits to optical and UV spectra,
we find evidence that in the case of AM CVn, we do not detect a
significant proportion of the accretion energy. This missing
component could be lost in the form of a wind.
Key words: accretion, accretion disks / stars: binaries: general / stars: novae: cataclysmic variables / X-rays: binaries / stars: individual: AM CVn, HP Lib, CR Boo, GP Com
© ESO, 2005
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