Population types of cataclysmic variables in the solar neighborhood

Ak, Tansel and Bilir, Selçuk and Güver, Tolga and Çakmak, Hikmet and Ak, Serap (2012) Population types of cataclysmic variables in the solar neighborhood. (Accepted/In Press)

WarningThere is a more recent version of this item available.

PDF (Preprint version of the accepted paper (This is a RoMEO green journal -- author can archive pre-print (ie pre-refereeing))) - Requires a PDF viewer such as GSview, Xpdf or Adobe Acrobat Reader

Official URL: http://dx.doi.org/10.1016/j.newast.2012.11.007


The Galactic orbital parameters of 159 cataclysmic variables in the Solar neighbourhood are calculated, for the first time, to determine their population types using published kinematical parameters. Population analysis shows that about 6 per cent of cataclysmic variables in the sample are members of the thi ck disc component of the Galaxy. This value is consistent with the fraction obt ained from star count analysis. The rest of the systems in the sample are found to be in the thin disc component of the Galaxy. Our analysis revealed no halo CVs in the Solar vicinity. About 60 per cent of the thick disc CVs have orbital periods be low the orbital period gap. This result is roughly consistent with the predictions of population synthesis models developed for cataclysmic variables. A kinematical age of 13 Gyr is obtained using total space velocity dispersion of the most probable thick disc CVs which is consistent with the age of thick disc component of the Galaxy.

Item Type:Article
Uncontrolled Keywords:97.80.Gm Cataclysmic binaries, 98.10.+z Stellar dynamics and kinematics, 98.35.Pr Solar neighbourhood
Subjects:Q Science > QB Astronomy
ID Code:21006
Deposited By:Tolga Güver
Deposited On:01 Dec 2012 22:52
Last Modified:31 Jul 2019 16:49

Available Versions of this Item

Repository Staff Only: item control page