Supernova 1996cr in ESO 97-G13 [with corrected sentence, re: Cbet 876]

Details Supernova 1996cr in ESO 97-G13 [with corrected sentence, re: Cbet 876] Supernova 1996cr in ESO 97-G13 [with corrected sentence, re: Cbet 876]

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007cbet..879...14b&link_type=abstract

Central Bureau Electronic Telegrams, 879, 14 (2007). Edited by Green, D. W. E.

Computer Science

Scientific paper

Radio data published by Elmouttie et al. (1998, MNRAS 297, 1202), and additional radio images at 3 and 6 cm (comprised of data taken between 1994 and 1996; Elmouttie, private communication), confirm that 1996cr has a faint (about 1- to 2-mJy) radio counterpart. From a radio light curve constructed by Bauer from ATCA-archive data, 1996cr begins to peak up above the noise by 1996 Dec. 5 (about 1-2 mJy). From the available data, it is unclear whether the peak of the radio emission has been reached yet; as of 2004 Apr. 2, 1996cr had the following radio-flux densities: 8.6 GHz, 162 mJy; 4.8 GHz, 240 mJy; 2.4 GHz, 364 mJy; 1.4 GHz, 481 mJy.

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