/ftp/cats/aliases/O/OCISM



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VII/106      Open Cluster Interstellar Matter Database   (Leisawitz 1988)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
	clusters.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=VII/106
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drwxr-xr-x 257 cats archive 8192 Feb 8 10:28 [Up] drwxr-xr-x 2 cats archive 4096 Jan 13 2023 [TAR file] -rw-r--r-- 1 cats archive 460 Dec 19 2022 .message -r--r--r-- 1 cats archive 3696 Aug 3 2004 ReadMe -rw-r--r-- 1 cats archive 356 Sep 24 2012 +footg5.gif -rw-r--r-- 1 cats archive 3027 Sep 24 2012 +footg8.gif -r--r--r-- 1 cats archive 6725 Aug 3 2004 clusters.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 363472 Oct 29 1998 ocdb.rec -r--r--r-- 1 cats archive 49647 Oct 29 1998 ocdb.ref -r--r--r-- 1 cats archive 44025 Oct 29 1998 ocdb_doc.txt -r--r--r-- 1 cats archive 212131 Oct 29 1998 ocdbmain.for -r--r--r-- 1 cats archive 746925 Aug 3 2004 ocism.lis
Beginning of ReadMe : VII/106 Open Cluster Interstellar Matter Database (Leisawitz 1988) =============================================================================== Open Cluster Interstellar Matter (OCISM) Database Leisawitz D.T. <NASA Ref. Publ. 1202 (1988)> =1988NASAR1202....1L ================================================================================ ADC_Keywords: Clusters, open ; Interstellar medium Description: This catalog is a compilation of the characteristics of 128 open clusters and the interstellar medium associated with them. It is distributed as the "OCISM Database" which is the set of data files, processing and analysis software written in FORTRAN, and the supporting documentation. As provided by the author, the data are in a multi-record format which is best accessed with the author's software. The clusters in this database have been relatively well-studied, have declinations greater than -20 deg., are between 1 and 5 kpc distant, and are younger than 100 million years old. Characteristics compiled for these clusters include cluster identification, spatial coordinates, radial velocities (of stellar clusters, H II regions, and molecular clouds), proper motions, distance, angular diameter, linear diameter, age, mass (based on stellar and atomic gas, ionized gas, molecular clouds, and dust determinations), visual extinction, and reddening.