Results 101 to 110 of about 5,465 (202)

Revisiting the Supernova Engines in the 3C 397 and W49B Supernova Remnants

The Astrophysical Journal
The nature of the supernova remnants (SNRs) 3C 397 and W49B has long been a subject of debate, with prior studies offering conflicting interpretations between thermonuclear and core-collapse scenarios. To help settle this debate, we present a systematic,
Cole Treyturik, Chelsea Braun, Samar Safi-Harb, Christopher L. Fryer, Gilles Ferrand   +4 more
doaj   +1 more source

Remnants of Stars Past - The Formation of Supernova Remnants

All stars die. Some stars die more violently than others. Supernovae occur when a star cannot resist the pull of gravity and collapses in on itself, causing a huge explosion to occur.
Tusler, Josiah
core  

Gamma-Ray Lines from Young Supernova Remnants

, 1969
The gamma-ray luminosity of a typical type I supernova remnant has been calculated by assuming that the origin of the optical luminosity is due to the energy of the radioactive decay of Ni56.
Clayton, Donald D, Fishman, Gerald J, Colgate, Stirling A   +2 more
core  

Single versus Binary Origin: The Diversity of Stripped-envelope Supernova Remnants

The Astrophysical Journal
Core-collapse supernova remnants (CCSNRs) are crucial for understanding the final stages of massive star evolution, as they reflect the imprints of their progenitors’ preexplosion activities.
Gaku Kawashima, Shiu-Hang Lee, Keiichi Maeda, Daniel Patnaude   +3 more
doaj   +1 more source

Neutron Stars in Supernova Remnants

, 2002
The grant provided funds for a conference entitled 'Neutron Stars in Supernova Remnants' held in Boston on 14-17 August 2001, in part to support invited speakers and students attending the meeting.
Kaluzienski, Lou, Slane, Patrick
core  

Relativistic electron acceleration at the bow shock of Jupiter and beyond. [PDF]

Nature
Raptis S, Turner DL, Caprioli D, Szalay JR, Clark G, Haggerty CC.   +5 more
europepmc   +1 more source

Using wavelet decomposition to determine the dimension of structures from projected images. [PDF]

Proc Natl Acad Sci U S A
Mayboroda S, Spergel DN.
europepmc   +1 more source

Simulations of multi-phase gas in and around galaxies. [PDF]

Living Rev Comput Astrophys
Gronke M, E Schneider E.
europepmc   +1 more source

Utilizing AI to unveil the nonlinear interplay of convection, drift, and diffusion on galactic cosmic ray modulation in the inner heliosphere. [PDF]

Sci Rep, 2022
Inceoglu F, Pacini AA, Loto'aniu PTM.
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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