SIMBAD references

2009A&A...496..805R - Astronomy and Astrophysics, volume 496, 805-812 (2009/3-4)

An evolved donor star in the long-period cataclysmic variable HS0218+3229.

RODRIGUEZ-GIL P., TORRES M.A.P., GAENSICKE B.T., MUNOZ-DARIAS T., STEEGHS D., SCHWARZ R., RAU A. and HAGEN H.-J.

Abstract (from CDS):

We present time-resolved spectroscopy and photometry of HS0218+3229, a new long-period cataclysmic variable discovered within the Hamburg Quasar Survey. It is one of the few systems that allow a dynamical measurement of the masses of the stellar components. We combine the analysis of time-resolved optical spectroscopy and R-band photometry with the aim of measuring the mass of the white dwarf and the donor star and the orbital inclination. Cross-correlation of the spectra with K-type dwarf templates is used to derive the radial velocity curve of the donor star. An optimal subtraction of the broadened templates is performed to measure the rotational broadening and constrain the spectral type of the donor. Finally, an ellipsoidal model is fitted to the R-band light curve to obtain constraints upon the orbital inclination of the binary system. The orbital period of HS0218+3229 is found to be 0.297229661±0.000000001d (7.13351186±0.00000002h), and the amplitude of the donor's radial velocity curve is K2=162.4±1.4km/s. Modelling the ellipsoidal light curves gives an orbital inclination in the range i=59°±3°. A rotational broadening between 82.4±1.2km/s and 89.4±1.3km/s is found when assuming zero and continuum limb darkening, respectively. The secondary star has most likely a spectral type K5 and contributes ∼80-85% to the R-band light. Our analysis yields a mass ratio of 0.52<q<0.65, a white dwarf mass of 0.44<M1(M)<0.65, and a donor star mass of 0.23<M2(M)<0.44. We find that the donor star in HS0218+3229 is significantly undermassive for its spectral type. It is therefore very likely that it has undergone nuclear evolution prior to the onset of mass transfer.

Abstract Copyright:

Journal keyword(s): accretion, accretion discs - stars: binaries: close - stars: novae, cataclysmic variables

Status at CDS:  

CDS comments: Fig.1 star C1 is 2MASS J02212369+3241290 in Simbad.

Simbad objects: 16

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2009A&A...496..805R and select 'bookmark this link' or equivalent in the popup menu


2020.06.03-03:31:19

© Université de Strasbourg/CNRS

    • Contact