/ftp/cats/J_other/ARA+A/42.685



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J/other/ARA+A/42.685      Young stars near the Sun           (Zuckerman+, 2004)
The following files can be converted to FITS (extension .fit or fit.gz)
	table?.dat
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Query from: http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/other/ARA+A/42.685
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drwxr-xr-x 4 cats archive 102 Jul 26 2011 [Up] drwxr-xr-x 2 cats archive 4096 May 26 2021 [TAR file] -rw-r--r-- 1 cats archive 472 Apr 2 2011 .message -r--r--r-- 1 cats archive 6839 Apr 2 2011 ReadMe -rw-r--r-- 1 cats archive 509 Apr 2 2011 +footg5.gif -rw-r--r-- 1 cats archive 3781 Apr 2 2011 +footg8.gif -r--r--r-- 1 cats archive 1621 Feb 7 2011 table1.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 2146 Feb 7 2011 table2.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 3189 Feb 7 2011 table3.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 1101 Feb 7 2011 table4.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 2407 Feb 7 2011 table5.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 1037 Feb 7 2011 table6.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/other/ARA+A/42.685 Young stars near the Sun (Zuckerman+, 2004) ================================================================================ Young stars near the Sun. Zuckerman B., Song I. <Annual Rev. Astron. Astrophys., 42, 685-721 (2004)> =2004ARA&A..42..685Z ================================================================================ ADC_Keywords: Stars, nearby ; YSOs ; Associations, stellar Abstract: Until the late 1990s the rich Hyades and the sparse UMa clusters were the only coeval, comoving concentrations of stars known within 60 pc of Earth. Both are hundreds of millions of years old. Then beginning in the late 1990s the TW Hydrae Association, the Tucana/Horologium Association, the beta Pictoris Moving Group, and the AB Doradus Moving Group were identified within  60pc of Earth, and the eta Chamaeleontis cluster was found at 97pc. These young groups (ages 8-50Myr), along with other nearby, young stars, will enable imaging and spectroscopic studies of the origin and early evolution of planetary systems.

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