Results 41 to 50 of about 13,120 (212)
A Most Energetic Type Ic Supernova: SN 2003L [PDF]
SummaryWe present extensive radio observations of SN2003L, the most luminous and energetic Type Ic radio supernova with the exception of SN 1998bw. Using radio data, we are able to constrain the physical parameters of the supernova, including the velocity and energy of the fastest ejecta, the temporal evolution of the magnetic field, and the density ...
openaire +4 more sources
ULTRA-BRIGHT OPTICAL TRANSIENTS ARE LINKED WITH TYPE Ic SUPERNOVAE [PDF]
16 pages, 4 figures, 1 table.
Pastorello, A. +43 more
openaire +6 more sources
Modeling Type Ic Supernovae with tardis: Hidden Helium in SN 1994I? [PDF]
Abstract Supernovae (SNe) with photospheric spectra devoid of hydrogen and helium features are generally classified as SNe Ic. However, there is ongoing debate as to whether helium can be hidden in the ejecta of SNe Ic (that is, helium is present in the ejecta, but produces no obvious features in the spectra).
Marc Williamson +2 more
openaire +2 more sources
SN 2005at − A neglected type Ic supernova at 10 Mpc [PDF]
We present a photometric and spectroscopic study of a reddened type Ic supernova (SN) 2005at. We report our results based on the available data of SN 2005at, including late-time observations from the Spitzer Space Telescope and the Hubble Space Telescope. In particular, late-time mid-infrared observations are something rare for type Ib/c SNe.
Kankare, E +9 more
openaire +4 more sources
A Search for Relativistic Ejecta in a Sample of ZTF Broad-lined Type Ic Supernovae
The dividing line between gamma-ray bursts (GRBs) and ordinary stripped-envelope core-collapse supernovae (SNe) is yet to be fully understood.
Alessandra Corsi +25 more
doaj +1 more source
Type Ia Supernovae: An Examination of Potential Progenitors and the Redshift Distribution [PDF]
We examine the possibility that supernovae type Ia (SN Ia) are produced by white dwarfs accreting from Roche-lobe filling evolved companions, under the assumption that a strong optically thick stellar wind from accretor is able to stabilize the mass ...
Canal R. +18 more
core +3 more sources
The Peculiar Type Ic Supernova 1997ef: Another Hypernova [PDF]
"To appear in the Astrophysical Journal, Vol.534 (2000)"
Iwamoto, K. +9 more
openaire +2 more sources
A `Hypernova' model for SN 1998bw associated with gamma-ray burst of 25 April 1998 [PDF]
The discovery of the peculiar supernova (SN) 1998bw and its possible association with the gamma-ray burst (GRB) 980425$^{1,2,3}$ provide new clues to the understanding of the explosion mechanism of very massive stars and to the origin of some classes of ...
Augusteijn, T. +26 more
core +1 more source
Discovery of a Relativistic Stripped-envelope Type Ic-BL Supernova at z = 2.83 with JWST
We present James Webb Space Telescope (JWST) NIRCam and NIRSpec observations of a Type Ic supernova (SN Ic) and its host galaxy (JADES-GS+53.13533-27.81457) at z = 2.83. This SN (named SN 2023adta) was identified in deep JWST/NIRCam imaging from the JWST
M. R. Siebert +28 more
doaj +1 more source
Critical Tests of Leading Gamma Ray Burst Theories
It has been observationally established that supernovae (SNe) of Type Ic produce long duration gamma-ray bursts (GRBs) and that neutron star mergers generate short hard GRBs.
Shlomo Dado +2 more
doaj +1 more source

