Results 21 to 30 of about 48,593 (219)

Comparing the Locations of Supernovae to CO (2–1) Emission in Their Host Galaxies

open access: yesThe Astrophysical Journal, 2023
We measure the molecular gas environment near recent (
Ness Mayker Chen   +21 more
doaj   +1 more source

The Effects of Thomson Scattering and Chemical Mixing on Early-time Light Curves of Double-peaked Type IIb Supernovae

open access: yesThe Astrophysical Journal, 2023
Previous numerical simulations of double-peaked Type IIb supernova (SN IIb) light curves have demonstrated that the radius and mass of the hydrogen-rich envelope of the progenitor star can significantly influence the brightness and timescale of the early-
Seong Hyun Park   +2 more
doaj   +1 more source

Type II Supernovae as Standardized Candles [PDF]

open access: yes, 2002
We present evidence for a correlation between expansion velocities of the ejecta of Type II plateau supernovae and their bolometric luminosities during the plateau phase. This correlation permits one to standardize the candles and decrease the scatter in
Barbon R.   +4 more
core   +3 more sources

SN 2019hcc: a Type II supernova displaying early O ii lines [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2021
ABSTRACT We present optical spectroscopy together with ultraviolet, optical, and near-infrared photometry of SN 2019hcc, which resides in a host galaxy at redshift 0.044, displaying a sub-solar metallicity. The supernova spectrum near peak epoch shows a ‘w’ shape at around 4000 Å which is usually associated with O ii lines and is typical
Eleonora Parrag   +20 more
openaire   +7 more sources

Inferencing Progenitor and Explosion Properties of Evolving Core-collapse Supernovae from Zwicky Transient Facility Light Curves

open access: yesThe Astrophysical Journal, 2023
We analyze a sample of 45 Type II supernovae from the Zwicky Transient Facility public survey using a grid of hydrodynamical models in order to assess whether theoretically driven forecasts can intelligently guide follow-up observations supporting all ...
Bhagya M. Subrayan   +11 more
doaj   +1 more source

SN 2018gk Revisited: the Photosphere, the Central Engine, and the Putative Dust

open access: yesThe Astrophysical Journal, 2023
We perform a comprehensive study of the physical properties of SN 2018gk, which is a luminous Type IIb supernova (SN). We find that the early-time photospheric velocity varies from a larger value to a smaller one before the photosphere reaches a ...
Tao Wang   +3 more
doaj   +1 more source

On Core Collapse Supernovae in Normal and in Seyfert Galaxies [PDF]

open access: yes, 2002
This paper estimates the relative frequency of different types of core-collapse supernovae, in terms of the ratio f between the number of type Ib--Ic and of type II supernovae.
Bressan, A.   +2 more
core   +2 more sources

Cosmology with Type II supernovae [PDF]

open access: yesInternational Journal of Modern Physics D, 2019
With the recent progresses on the Type II supernovae, we attempt to investigate whether there does exist new physics beyond the standard cosmological paradigm, i.e. the cosmological constant [Formula: see text] plus cold dark matter ([Formula: see text]CDM).
openaire   +2 more sources

Carnegie Supernova Project-II: Near-infrared Spectroscopic Diversity of Type II Supernovae [PDF]

open access: yesThe Astrophysical Journal, 2019
AbstractWe present 81 near-infrared (NIR) spectra of 30 Type II supernovae (SNe II) from theCarnegie Supernova Project-II(CSP-II), the largest such data set published to date. We identify a number of NIR features and characterize their evolution over time. The NIR spectroscopic properties of SNe II fall into two distinct groups.
S. Davis   +26 more
openaire   +5 more sources

Progenitors of Type IIb Supernovae. II. Observable Properties [PDF]

open access: yesThe Astrophysical Journal, 2020
Abstract Type IIb supernovae (SNe IIb) present a unique opportunity for investigating the evolutionary channels and mechanisms governing the evolution of stripped-envelope SN progenitors due to a variety of observational constraints.
Niharika Sravan   +4 more
openaire   +3 more sources

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