/ftp/cats/J_BaltA/17/1



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J/BaltA/17/1        GL490 region infrared photometry         (Straizys+, 2008)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
	table1.dat table2.dat table3.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/BaltA/17/1
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drwxr-xr-x 6 cats archive 124 Jan 29 2012 [Up] drwxr-xr-x 2 cats archive 308 Jan 13 2023 [TAR file] -rw-r--r-- 1 cats archive 490 Dec 19 2022 .message -r--r--r-- 1 cats archive 7124 Aug 14 2008 ReadMe -rw-r--r-- 1 cats archive 1006 Nov 13 2012 +footg5.gif -rw-r--r-- 1 cats archive 2201 Nov 13 2012 +footg8.gif -r--r--r-- 1 cats archive 2954 Jul 29 2008 table1.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 1429 Jul 29 2008 table2.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 4488 Jul 5 2008 table3.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/BaltA/17/1 Infrared photometry in GL490 star-forming region (Straizys+ 2008) ================================================================================ Young stars in the Camelopardalis dust and molecular clouds. III. The GL490 region. Straizys V., Laugalys V. <Baltic Astron. 17, 1-19 (2008)> =2008BaltA..17....1S ================================================================================ ADC_Keywords: Clusters, open ; Photometry, infrared Keywords: stars: formation - stars: pre-main sequence - infrared: stars - ISM: dust, extinction, clouds - Galaxy: open clusters and associations: individual (Cam OB1) Abstract: Using the infrared photometry data extracted from the 2MASS, IRAS and MSX databases, 50 suspected young stellar objects (YSOs) are selected from about 37500 infrared objects in the 3x3deg^2^ area with the center at (l,b=142.5,+1.0), in the vicinity of the young stellar object GL 490 in the dark cloud T 942 (Dobashi et al., 2005PASJ...57S...1D, Cat. VII/244). The spectral energy distributions between 700nm and 100um suggest that most of the selected objects may be YSOs of classes I and II. In the color-magnitude diagram Ks vs. H-Ks the suspected YSOs occupy an area right of the main sequence what can be interpreted as being caused by the effects of luminosity, interstellar and circumstellar reddening and infrared thermal emission in circumstellar envelopes and disks.