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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.cds.unistra.fr/viz-bin/VizieR?-source=J/other/ARA+A/42.685
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-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]
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Beginning of ReadMe :J/other/ARA+A/42.685 Young stars near the Sun (Zuckerman+, 2004)
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Young stars near the Sun.
Zuckerman B., Song I.
<Annual Rev. Astron. Astrophys., 42, 685-721 (2004)>
=2004ARA&A..42..685Z
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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.