Search for and Identification of Young Compact Galactic Supernova Remnants Using THOR [PDF]
S. Ranasinghe, D. A. Leahy, J. M. Stil
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The Binary Fraction of B-type Runaway Stars from LAMOST DR8
Runaway stars are defined as stars that depart from their birth clusters at high peculiar velocities. There are two main mechanisms for the formation of runaway stars, i.e., the binary-supernova scenario (BSS) and the dynamical ejection scenario (DES ...
Kun Chen +4 more
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Determining the main-sequence mass of Type II supernova progenitors [PDF]
Luc Dessart, Eli Livne, Roni Waldman
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The Relation between Helium White Dwarf Mass and Orbital Period under Two Types of Opacity
Helium white dwarfs (He WDs) are end products of low-mass red giant donors in close binary systems via stable mass transfer or common envelope evolution.
Jian Mou +7 more
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Type II Supernova Spectral Diversity. II. Spectroscopic and Photometric Correlations [PDF]
Claudia P. Gutiérrez +9 more
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Near-critical supernova outflows and their neutrino signatures
A. Friedland, Payel Mukhopadhyay
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Dips in the diffuse supernova neutrino background [PDF]
Yasaman Farzan +3 more
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Interacting supernovae and supernova impostors: Evidence of incoming supernova explosions? [PDF]
Violent eruptions, and consequently major mass loss, are a common feature of the so–called Luminous Blue Variable (LBV) stars. During major eruptive episodes LBVs mimic the behavior of real type IIn supernovae (SNe), showing comparable radiated energy and similar spectroscopic properties.
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Supernova Burst and Diffuse Supernova Neutrino Background Simulator for Water Cherenkov Detectors
If a Galactic core-collapse supernova explosion occurs in the future, it will be critical to rapidly alert the community to the direction of the supernova by utilizing neutrino signals in order to enable the initiation of follow-up optical observations ...
Fumi Nakanishi +3 more
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Charged-Current Neutrino-Nucleus Scattering off the Even Molybdenum Isotopes
Neutrinos from supernovae constitute important probes of both the currently unknown supernova mechanisms and of neutrino properties. Reliable information about the nuclear responses to supernova neutrinos is therefore crucial.
E. Ydrefors, J. Suhonen
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