/ftp/cats/J_A+A/339/./123



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J/A+A/339/123       PSR J1012+5307 evolutionary tracks (Driebe+ 1998)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
	table*.dat
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Query from: http://vizier.cds.unistra.fr/cgi-bin/VizieR?-source=J/A+A/339/123
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drwxr-xr-x 7 cats archive 140 Jan 29 2012 [Up] drwxr-xr-x 2 cats archive 4096 Jan 12 2023 [TAR file] -rw-r--r-- 1 cats archive 460 Dec 19 2022 .message -r--r--r-- 1 cats archive 3537 Nov 3 1998 ReadMe -rw-r--r-- 1 cats archive 213 Sep 19 2007 +footg5.gif -rw-r--r-- 1 cats archive 2047 Mar 5 2008 +footg8.gif -r--r--r-- 1 cats archive 84764 Oct 8 1998 table10.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 98032 Oct 8 1998 table11.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 76961 Oct 8 1998 table5.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 83261 Oct 8 1998 table6.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 178837 Oct 8 1998 table7.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 127075 Oct 8 1998 table8.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 79768 Oct 8 1998 table9.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/A+A/339/123 PSR J1012+5307 evolutionary tracks (Driebe+ 1998) ================================================================================ The evolution of helium white dwarfs. I. The companion of the millisecond pulsar PSR J1012+5307 Driebe T., Schoenberner D., Bloeckera T., Herwig F. <Astron. Astrophys. 339, 123 (1998)> =1998A&A...339..123D (SIMBAD/NED BibCode) ================================================================================ ADC_Keywords: Stars, dwarfs; Pulsars ; Models, evolutionary Keywords: stars: evolution - stars: interiors - stars: white dwarfs binaries: general - pulsars: individual: PSR J1012+5307 Description: We present a set of evolutionary tracks for white dwarfs with helium cores in the mass range from 0.179 to 0.414M_sun_. The tracks are based on a 1M_sun_ model sequence extending from the pre-main sequence stage up to the tip of the red-giant branch. Applying large mass loss rates at appropriate positions forced the models to move off the giant branch.The further evolution was then followed across the Hertzsprung-Russell diagram and down the cooling branch. Objects: ---------------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------------- 10 12 33.5 +53 07 03 PSR J1012+5307 = PSR J1012+53 ----------------------------------------------------------