Abstract M. Hamuy and M. Phillips, Carnegie Observatories; N. Suntzeff, Cerro Tololo Inter- American Observatory; and J. Maza, University of Chile, report that spectroscopic …
J Deng, KS Kawabata, Y Ohyama… - The Astrophysical …, 2004 - iopscience.iop.org
Optical spectroscopy of the Type Ia supernova SN 2002ic obtained on 2003 June 27.6 UT, ie,∼ 222 rest-frame days after explosion, is presented. Strong H emission indicates an …
J Parrent, D Branch, MA Troxel… - Publications of the …, 2007 - iopscience.iop.org
Synthetic spectra generated with the parameterized supernova synthetic spectrum code SYNOW are compared to spectra of the unusual Type Ib supernova 2005bf. We confirm the …
S Justham - The Astrophysical Journal Letters, 2011 - iopscience.iop.org
The lack of hydrogen in spectra of type Ia supernovae (SNe Ia) is often seen as troublesome for single-degenerate (SD) progenitor models. We argue that, since continued accretion of …
JM Silverman, P Mazzali, R Chornock… - Publications of the …, 2009 - iopscience.iop.org
Here we present previously unpublished optical spectra of supernova (SN) 2001ig, a Type IIb SN, from about a week after explosion until nearly one year later. The earliest spectrum …
We present the first unambiguous detection of helium emission lines in spectra of Type Ic supernovae (SNe Ic). The presence of He I lines with FWHM≈ 2000 km s-1 and the distinct …
SN 2017dio shows both spectral characteristics of a type-Ic supernova (SN) and signs of a hydrogen-rich circumstellar medium (CSM). Prominent, narrow emission lines of H and He …
An optical photometric and spectroscopic analysis of the slowly-evolving type IIn SN 2007rt is presented, covering a duration of 481 days after discovery. Its earliest spectrum, taken …
We report spectroscopic and photometric observations of the Type IIb SN 2011dh obtained between 4 and 34 days after the estimated date of explosion (May 31.5 UT). The data cover …