Results 101 to 110 of about 809 (163)

The liminal position of Nuclear Physics: from hadrons to neutron stars. [PDF]

Philos Trans A Math Phys Eng Sci
Petri M, Gezerlis A.
europepmc   +1 more source

Information-Entropy Analysis of Stellar Evolutionary Stages with Application to FS CMa Objects. [PDF]

Entropy (Basel)
Zhanabaev Z, Akniyazova A, Ashimov Y.
europepmc   +1 more source

Neutrino communication, intergalactic transit, and Astrobiology. [PDF]

Bioinformation, 2022
Shapshak P.
europepmc   +1 more source

Proton Acceleration with Relativistic Electromagnetic Shock. [PDF]

Adv Sci (Weinh)
Xiao T, Zhang X, Kong F, Zheng X, Gong Z, Shen B.   +5 more
europepmc   +1 more source

Supernova dust destruction in the magnetized turbulent ISM. [PDF]

Nat Commun
Kirchschlager F, Mattsson L, Gent FA.
europepmc   +1 more source

A connection between proto-neutron-star Tayler-Spruit dynamos and low-field magnetars. [PDF]

Nat Astron
Igoshev A, Barrère P, Raynaud R, Guilet J, Wood T, Hollerbach R.   +5 more
europepmc   +1 more source

Evolution of Supernova Remnants. I. Interacting Supernova Remnants

Evolution of Supernova Remnants. I. Interacting Supernova Remnants
application ...
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Multiple outflows and delayed ejections revealed by early imaging of novae. [PDF]

Nat Astron
Aydi E, Monnier JD, Mérand A, Schaefer GH, Chomiuk L, Otulakowska-Hypka M, Fan JL, Li KL, Sokolovsky KV, Salinas R, Tucker M, Shappee B, Rudy R, Page KL, Kuin NPM, Buckley DAH, Craig P, Izzo L, Linford J, Metzger BD, Mukai K, Orio M, Shen KJ, Strader J, Sokoloski JL, Williams RE, Williams MN, Habtie GR, Kraus S, Anugu N, Bouquin JL, Chhabra S, Codron I, Gardner T, Gutierrez M, Ibrahim N, Lanthermann C, Setterholm BR, Ashall C, Hinkle JT, Jaeger T, Payne AV.   +41 more
europepmc   +1 more source

Inner Workings: Physicists look to a new telescope to understand neutron stars and matter at the extremes. [PDF]

Proc Natl Acad Sci U S A, 2020
Ornes S.
europepmc   +1 more source

Evolution of Supernova Remnants. 1. Interacting Supernova Remnants

Evolution of Supernova Remnants. 1. Interacting Supernova Remnants
application/pdf The evolution and structure of two interacting supernova remnants (SNRS) are calculated by use of a timedependent two-dimensional hydro- dynamic code. The interactions of two SNRs are simulated in such a Way that at a time t。 after the first supernova explosion, the second Supernova explosion occurs at the distance D and two SNRs ...
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