Fv. Hessman et al., THE ECLIPSING AM HERCULIS BINARY V2301 OPHIUCHI .1. ROSAT AND IUE OBSERVATIONS, Astronomy and astrophysics, 327(1), 1997, pp. 245-251
We present X-ray and UV observations of the unique eclipsing cataclysm
ic variable V2301 Oph (1H1752+081). The X-ray eclipse of the primary s
tar is total and corresponds in phase with the optical eclipse of the
white dwarf. The X-ray light curve shows a quasi-sinusoidal orbital ''
hump'' typical of AM Her systems. The orbital phase at which the hump
has its peak has remained at similar to 0.9 in all ROSAT observations
taken over several years. We can rule out a 100% modulated spin-pulse
signal with a period shorter than P-orb. Thus, it is very unlikely tha
t there is either a non-synchronously rotating white dwarf or an accre
tion disk in V2301 Oph. The relatively hard X-ray spectrum of this wea
kly-magnetic system does not change its shape during the orbit or arou
nd the eclipse and is consistent with that expected from a hot accreti
on column on a weakly magnetized white dwarf. The interstellar absorbi
ng column density of similar to 4.10(20) H-atoms cm(-2) required by th
e X-ray spectral fits is capable of hiding any weak soft X-ray compone
nt. The lower limit to the relative contributions of a hard bremsstrah
lung and a soft blackbody component is consistent with both the empiri
cal relation for AM Hers and the theoretical expectations for a system
with a low magnetic field strength. The irregular ''dips'' present in
the light curve around phases 0.85-0.92 with depths up to 80% are not
accompanied by significant changes in the hardness ratios and must be
due to partial covering by a structured and blobby accretion stream w
hich has been lifted out of the orbital plane by the magnetic field of
the primary. The close agreement between the phasing of the dips and
the peak of the X-ray light curves is expected in a synchronous magnet
ic accretor. The relative strengths of the NV, CIV, and Hell UV emissi
on lines are typical for AM Her stars. Thus, the X-ray orbital light c
urves and the X-ray and UV spectra clearly identify V2301 Oph as an AM
Her system.