Results 91 to 100 of about 7,219,823 (215)
Optical Spectroscopy of Type Ib/c Supernovae
Accepted for publication in the March issue of AJ.
Matheson, Thomas +4 more
openaire +2 more sources
Type Ib and Ic supernovae: Models and spectra
In this paper we consider the properties of massive star models for type Ib and Ic supernovae. There are two ways that a massive star can lose its hydrogen envelope - binary mass exchange and stellar wind. These are not mutually exclusive.
Woosley, S.E. (California Univ., Santa Cruz, CA (United States). Board of Studies in Astronomy and Astrophysics +3 more
core
Optical Spectra of Thermonuclear Supernovae in the Local and Distant Universe [PDF]
This thesis is devoted to the study of optical spectra of thermonuclear supernovae, known as ``Type Ia'' supernovae (SN Ia). These violent stellar explosions, visible across a large fraction of the observable universe, are used to measure distances on ...
Blondin, Stephane
core +1 more source
Spectropolarimetric Evolution Reveals Dual-axis Ejecta in the Atypical Magnetar-powered SN 2012au
We present six epochs of optical spectropolarimetric observations of the unique and slow-evolving Type Ib supernova (SN) 2012au, between 0 and 295 day post- R -band maximum.
Sabrina DeSoto +9 more
doaj +1 more source
Eruptive mass loss of massive stars prior to supernova (SN) explosion is key to understanding their evolution and end fate. An observational signature of pre-SN mass loss is the detection of an early, short-lived peak prior to the radioactive-powered ...
Kaustav K. Das +36 more
doaj +1 more source
SN 2023zaw: The Low-energy Explosion of an Ultrastripped Star
Most stripped-envelope supernova progenitors are thought to be formed through binary interaction, losing hydrogen and/or helium from their outer layers. Ultrastripped supernovae are an emerging class of transient that are expected to be produced through ...
T. Moore +28 more
doaj +1 more source
Nonthermal excitation of helium in type Ib supernovae
The presence of strong He I absorption troughs in the optical spectra of type Ib SNs is attributed to non-thermal excitation. As for analogous in the premaximum spectra of SN 1987A, the early importance of nonthermal excitation in the Ib's is fundamentally due to a large-scale instability that mixes 56 Ni out into their envelopes shortly after the ...
openaire +1 more source
Observational constraints on the progenitor metallicities of core-collapse supernovae [PDF]
Artículo de publicación ISIWe present constraints on the progenitor metallicities of core-collapse supernovae. To date, nearly all metallicity constraints have been inferred from indirect methods such as metallicity gradients in host galaxies ...
James, P. A. +9 more
core +1 more source
Absolute Magnitude Distributions and Light Curves of Stripped-Envelope Supernovae [PDF]
The absolute visual magnitudes of three Type IIb, 11 Type Ib, and 13 Type le supernovae (collectively known as stripped-envelope supernovae) are studied by collecting data on the apparent magnitude, distance, and interstellar extinction of each event ...
Branch, D., Richardson, D., Baron, E.
core +1 more source
We present optical and near-infrared (NIR) observations of the Type Ib supernova (SN) 2024rbc. Emission from the first CO overtone, resting on a dust continuum at 2.3−2.4 μ m, was observed at 62 days postexplosion. The CO band heads are not resolved, and
Ryan Hwangbo +18 more
doaj +1 more source

