Supernovae 2004bu, 2004bw, 2004bz, 2004cb, and 2004cc

Details Supernovae 2004bu, 2004bw, 2004bz, 2004cb, and 2004cc Supernovae 2004bu, 2004bw, 2004bz, 2004cb, and 2004cc

Jun 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004iauc.8353....2m&link_type=abstract

IAU Circ., 8353, 2 (2004). Edited by Green, D. W. E.

Astronomy and Astrophysics

Astrophysics

2

Scientific paper

T. Matheson, P. Challis, and R. Kirshner, Harvard-Smithsonian Center for Astrophysics, report that a spectrum (range 340-730 nm) of SN 2004cc (cf. IAUC 8350), obtained by K. Penev on June 10.46 UT with the F. L. Whipple Observatory 1.5-m telescope (+ FAST spectrograph), shows it to be a supernova, most likely of type I, but the exact classification is uncertain. The spectrum appears to be highly reddened (a Na I D absorption at the host velocity has an equivalent width of 0.44 nm). There are peaks near 540 and 580 nm and absorptions near 560 and 630 nm.

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