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II/289 LDN 1688 JKH photometry (Wilking+, 2008)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
table1.dat refs.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=II/289
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drwxr-xr-x 351 cats archive 8192 Mar 25 10:13 [Up]
drwxr-xr-x 3 cats archive 4096 Jan 12 2023 [TAR file]
-rw-r--r-- 1 cats archive 472 Dec 19 2022 .message
-r--r--r-- 1 cats archive 8264 Jan 25 2016 ReadMe
-rw-r--r-- 1 cats archive 1004 Mar 7 2016 +footg5.gif
-rw-r--r-- 1 cats archive 2320 Mar 7 2016 +footg8.gif
-r--r--r-- 1 cats archive 1888 Dec 9 2008 refs.dat [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 76470 Mar 7 2016 table1.dat [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 13049 Dec 9 2008 table1.v00.gz [Uncompressed]
-r--r--r-- 1 cats archive 76470 Mar 7 2016 table1.v01 Beginning of ReadMe :II/289 JKH photometry in LDN 1688 (Wilking+, 2008)
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Star Formation in the rho Ophiuchi Molecular Cloud.
Wilking B.A., Gagne M., Allen L.E.
<Astron. Soc. Pac. Monograph Publications, 5, 351-380 (2008)>
=2008yCat.2289....0W
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ADC_Keywords: Molecular clouds ; Photometry, infrared ; Cross identifications
Abstract:
A review of star formation in the Rho Ophiuchi molecular complex is
presented, with particular emphasis on studies of the main cloud,
L1688, since 1991. Recent photometric and parallax measurements of
stars in the Upper Scorpius subgroup of the Sco-Cen OB association
suggest a distance for the cloud between 120 and 140 parsecs. Star
formation is ongoing in the dense cores of L1688 with a median age for
young stellar objects of 0.3Myr. The surface population appears to
have a median age of 2-5Myr and merges with low mass stars in the
Upper Scorpius subgroup. Making use of the most recent X-ray and
infrared photometric surveys and spectroscopic surveys of L1688, we
compile a list of over 300 association members with counterparts in
the 2MASS catalog. Membership criteria, such as lithium absorption,
X-ray emission, and infrared excess, cover the full range of
evolutionary states for young stellar objects. Spectral energy
distributions are classified for many association members using
infrared photometry obtained from the Spitzer Space Telescope.