Computational investigation of spin-resolved energy landscapes of FeC<sub>4</sub>H<sub>2</sub> <sup>+</sup> and their astrochemical implications. [PDF]
Front ChemShajan S, Thirumoorthy K.
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Binary progenitor systems for Type Ic supernovae. [PDF]
Nat CommunSolar M +20 more
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Shock-induced nucleation of nanophase Fe-Ni alloy and its implications for interstellar iron reservoirs. [PDF]
Front ChemVelampatti Selvaraj P, Chandrasekaran V.
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Modeling of Light Curves from Core Collapse Supernovae
Supernovae are known to astronomers for more than a thousand years, but their gravitational waves have never been detected, even though they\u27re expected to carry a great wealth of information which could not be obtained in any other way.
Wall, Katelynn, Markovsky, Jake
core
False positives in gravitational wave campaigns: the electromagnetic perspective. [PDF]
Philos Trans A Math Phys Eng SciOates S.
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Strong Gravitational Lensing and Microlensing of Supernovae. [PDF]
Space Sci RevSuyu SH +4 more
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Understanding the Neutrino Dynamics in Pre-Core Collapse Supernovae
Core-collapse supernovae represent some of the most energetic events in the universe, where neutrino interactions play a crucial role in the explosion mechanism.
Bhat, Yash
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Increased and varied radiation during the Sun's encounters with cold clouds in the last 10 million years. [PDF]
Sci RepOpher M +9 more
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Inner Workings: A massive star dies without a bang, revealing the sensitive nature of supernovae. [PDF]
Proc Natl Acad Sci U S A, 2020 Croswell K.
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The Explosion and Progenitor Properties of Type IIP Supernovae Inferred from MESA and STELLA Modelling. [PDF]
Res Notes AAS, 2020 Ricks W, Dwarkadas VV.
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