Results 61 to 70 of about 695 (169)

Magnetorotational Mechanism of Supernova Type II Explosion

open access: yesInternational Astronomical Union Colloquium, 2005
SummaryResults of 2D simulations of the magnetorotational mechanism of supernova type II are presented. Amplification of toroidal magnetic field of the star due to differential rotation of the star leads to the transformation of the rotational (gravitational) energy to the energy of the supernova explosion. In our simulation the energy of the explosion
Moiseenko, S. G.   +2 more
openaire   +2 more sources

Physical properties of long-rising type II supernovae

open access: yesAstronomy & Astrophysics
Context. The supernova (SN) 1987A, with its long-rising (≳40 days) light curve, defines a rare subclass of type II SNe known as 1987A-like events. Representing only ∼1–3% of all core-collapse SNe and often found in low-metallicity environments, their ...
Cosentino S. P., Inserra C., Pumo M. L.
doaj   +1 more source

SN 2024abfl: A Flat-plateau, Low-luminosity Type IIP Supernova with Early Circumstellar Matter Interaction

open access: yesThe Astrophysical Journal
We present photometric and spectroscopic observations of SN 2024abfl, a low-luminosity Type IIP supernova (LLSN) discovered shortly after explosion. The transient reached a peak absolute magnitude of M _V  = −14.9 and exhibited an extended, flat plateau ...
Madison Gerard   +33 more
doaj   +1 more source

A Natural ≳100× Telescope: Discovery of the Strongly Lensed Type II SN 2025mkn at z = 1.37

open access: yesThe Astrophysical Journal Letters
We present the discovery of SN 2025mkn, a gravitationally lensed Type II supernova. First detected as a blue transient in Zwicky Transient Facility (ZTF), 0 $\mathop{.}\limits{^{\prime\prime} }$ 83 from a z = 0.42 elliptical galaxy, the follow-up SNIFS ...
Cameron Lemon   +92 more
doaj   +1 more source

A Type II Supernovae Constraint on $ν_e$-$ν_s$

open access: yes, 1993
plain Tex 11 pages, 3 figures available upon request from the authors. (shi6@oddjob.uchicago.edu, sigl@oddjob)
Shi, Xiangdong, Sigl, Guenter
openaire   +2 more sources

Spectropolarimetry of Type II supernovae

open access: yesAstronomy & Astrophysics
The explosion processes of supernovae (SNe) are imprinted in their explosion geometries. The recent discovery of several highly aspherical core-collapse SNe is significant, and studying these is regarded as being crucial in order to understand the underlying explosion mechanism.
Nagao, T.   +8 more
openaire   +4 more sources

Final Moments. III. Explosion Properties and Progenitor Constraints of CSM-interacting Type II Supernovae

open access: yesThe Astrophysical Journal
We present analysis of the plateau and late-time phase properties of a sample of 39 Type II supernovae (SNe II) that show narrow, transient, high-ionization emission lines (i.e., “IIn-like”) in their early-time spectra from interaction with confined ...
W. V. Jacobson-Galán   +54 more
doaj   +1 more source

SN 2022jox: An Extraordinarily Ordinary Type II SN with Flash Spectroscopy

open access: yesThe Astrophysical Journal
We present high-cadence optical and ultraviolet (UV) observations of the Type II supernova (SN), SN 2022jox which exhibits early spectroscopic high-ionization flash features of H i , He ii , C iv , and N iv that disappear within the first few days after ...
Jennifer E. Andrews   +22 more
doaj   +1 more source

Discovery of a Variable Yellow Supergiant Progenitor for the Type IIb SN 2024abfo

open access: yesThe Astrophysical Journal Letters
We report the discovery of a progenitor candidate for the Type IIb SN 2024abfo using multiepoch pre-explosion images from the Hubble Space Telescope and the Dark Energy Camera Legacy Survey.
Zexi Niu   +6 more
doaj   +1 more source

Discovery of a Dusty Yellow Supergiant Progenitor for the Type IIb SN 2017gkk

open access: yesThe Astrophysical Journal Letters
Type IIb supernovae are an important subclass of stripped-envelope supernovae (SNe), which show H lines only at early times. Their progenitors are believed to contain a low-mass H envelope before explosion. This work reports the discovery of a progenitor
Zexi Niu, Ning-Chen Sun, Jifeng Liu
doaj   +1 more source

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