========================================================================== J/AJ/127/1632 UBVR(UIT) photometry of O and OB stars in SMC (Oey+, 2004) The following files can be converted to FITS (extension .fit .fgz or .fiZ) table2.dat table3.dat table[45].dat ========================================================================== Query from: http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/AJ/127/1632 ==========================================================================
drwxr-xr-x 76 cats archive 4096 Jan 29 2012 [Up] drwxr-xr-x 2 cats archive 4096 Jun 16 10:59 [TAR file] -rw-r--r-- 1 cats archive 494 Feb 20 2005 .message -r--r--r-- 1 cats archive 4700 Feb 20 2005 ReadMe -rw-r--r-- 1 cats archive 1016 Sep 19 2007 +footg5.gif -rw-r--r-- 1 cats archive 2603 Mar 5 2008 +footg8.gif -r--r--r-- 1 cats archive 4884 Oct 21 2004 table2.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 1276 Oct 21 2004 table3.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 115600 Oct 21 2004 table4.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 32088 Oct 21 2004 table5.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/AJ/127/1632 UBVR(UIT) photometry of O and OB stars in SMC (Oey+, 2004) ================================================================================ Massive field stars and the stellar clustering law. Oey M.S., King N.L., Parker J.W. <Astron. J., 127, 1632-1643 (2004)> =2004AJ....127.1632O ================================================================================ ADC_Keywords: Magellanic Clouds ; Photometry, UBVRI Keywords: galaxies: star clusters - galaxies: stellar content - Magellanic Clouds - stars: early-type - stars: formation - stars: statistics Abstract: The distribution of N*, the number of OB stars per association or cluster, appears to follow a universal power-law form (N*)^-2^ in the local universe. We evaluate the distribution of N* in the Small Magellanic Cloud using recent broadband optical and space-ultraviolet data, with special attention to the lowest values of N*. We find that the power-law distribution in N* continues smoothly down to N*=1. This strongly suggests that the formation of field massive stars is a continuous process with those in associations and that the field stars do not originate from a different star formation mode.
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