/ftp/cats/J_other/NewA/34.234



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J/other/NewA/34.234 Galactic cataclysmic variables distances   (Ozdonmez+, 2015)
The following files can be converted to FITS (extension .fit or fit.gz)
	catalog.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/other/NewA/34.234
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drwxr-xr-x 60 cats archive 4096 Mar 29 2023 [Up] drwxr-xr-x 4 cats archive 4096 Jan 13 2023 [TAR file] -rw-r--r-- 1 cats archive 475 Dec 19 2022 .message -r--r--r-- 1 cats archive 4210 Aug 19 2015 ReadMe -rw-r--r-- 1 cats archive 609 Jul 16 2020 +footg5.gif -rw-r--r-- 1 cats archive 5605 Jul 16 2020 +footg8.gif -r--r--r-- 1 cats archive 29735 Jul 16 2020 catalog.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/other/NewA/34.234 Galactic cataclysmic variables distances (Ozdonmez+, 2015) ================================================================================ Galactic model parameters of cataclysmic variable: Results from a new absolute magnitude calibration with 2MASS and WISE. Ozdonmez A., Ak T., Bilir S. <New Astron., 34, 234-244 (2015)> =2015NewA...34..234O ================================================================================ ADC_Keywords: Stars, nearby ; Binaries, cataclysmic ; Stars, distances Keywords: stars: cataclysmic variables -stars: luminosity function - Galaxy: solar neighbourhood Abstract: In order to determine the spatial distribution, Galactic model parameters and luminosity function of cataclysmic variables (CVs), a J-band magnitude limited sample of 263 CVs has been established using a newly constructed period-luminosity-colours (PLCs) relation which includes J,KsJ,Ks and W1W1-band magnitudes in 2MASS and WISE photometries, and the orbital periods of the systems. This CV sample is assumed to be homogeneous regarding to distances as the new PLCs relation is calibrated with new or re-measured trigonometric parallaxes. Description: The data sample used in construction of the new PLCs relation consists of CVs in Table 1 including their classes, orbital periods (Porb), trigonometric parallaxes (pi) relative parallax errors (sigma_pi/pi), 2MASS J and Ks magnitudes and WISE W1 magnitudes.