Journal
ASTRONOMY & ASTROPHYSICS
Volume 471, Issue 2, Pages 527-U60Publisher
EDP SCIENCES S A
DOI: 10.1051/0004-6361:20066971
Keywords
stars : supernovae : general; stars : supernovae : individual : SN 2005cf
Categories
Ask authors/readers for more resources
The ESC-RTN optical spectroscopy data set for SN 2005cf is presented and analyzed. The observations range from -11.6 and + 77.3 days with respect to B-band maximum light. The evolution of the spectral energy distribution of SN 2005cf is characterized by the presence of high velocity Si II and Ca II features. SYNOW synthetic spectra are used to investigate the ejecta geometry of silicon. Based on the synthetic spectra, the Si II high-velocity feature appears detached at 19 500 km s(-1). We also securely establish the presence of such a feature in SN 1990N, SN 1994D, SN 2002er, and SN 2003du. In a morphological study both the Ca II IR triplet and H&K absorption lines of SN 2005cf show high-velocity features centered around 24 000 km s(-1). When compared with other type Ia SNe based on the scheme presented in Benetti et al. ( 2005, ApJ, 623, 1011), SN 2005cf definitely belongs to the LVG group.
Authors
I am an author on this paper
Click your name to claim this paper and add it to your profile.
Reviews
Recommended
No Data Available