/ftp/cats/7/210



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VII/210   ==OBSOLETE version of Catalogue==
28-Nov-1998: See VII/211
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=VII/210
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drwxr-xr-x 257 cats archive 8192 Feb 8 10:28 [Up] drwxr-xr-x 2 cats archive 211 May 26 2023 [TAR file] -rw-r--r-- 1 cats archive 369 Dec 19 2022 .message -rw-r--r-- 1 cats archive 25 Nov 28 1998 =obsolete= -r--r--r-- 1 cats archive 7605 Jul 23 1998 ReadMe -r--r--r-- 1 cats archive 13738 Jul 23 1998 snrs.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 27092 Jul 23 1998 snrs.doc
Beginning of ReadMe : VII/210 A Catalogue of Galactic Supernova Remnants (Green, 1996) ================================================================================ A Catalogue of Galactic Supernova Remnants, 1996 August version Green D.A. <in Supernovae and Supernova Remnants, the proceedings IAU Colloquium 145, eds McCray R. & Wang Z., Cambridge University Press, p. 419 (1996)> =1996IAUCo.145..419G ================================================================================ ADC_Keywords: Supernova remnants ; Milky Way ; Nonstellar objects Abstract: This catalog of known Galactic supernova remnants (SNRs) is an updated version (Version VI, August 1996) of the catalogs of Galactic SNRs presented in detail in Green (Version I 1984, Version II 1988), in summary form in Green (Version III 1991, Version IV 1996), and on the Web (Version V, July 1995). (Note that Version IV, although published in 1996, was producted in 1993.) This August 1996 version of the catalog contains 215 SNRs, which is 21 more than listed in the previous version. The basic summary data included in this catalog for each SNR are its Galactic coordinates, RA and Dec (B1950.0), angular size (in arcmin), type, flux density at 1 GHz, spectral index, and any other names. Notes on these parameters, on possible remnants not included, and questionable SNRs listed in the catalog are given in the documentation file (snrs.doc). It should be noted that there are serious selection effects which apply to the identification of Galactic SNRs (see Green 1991), so that great care should be taken if these data are used in statistical studies.