Results 241 to 250 of about 167,251 (265)

Evidence from stable isotopes and ¹⁰Be for solar system formation triggered by a low-mass supernova. [PDF]

Nat Commun, 2016
Banerjee P, Qian YZ, Heger A, Haxton WC.
europepmc   +1 more source

A detailed X-ray and radio comparison of Kepler's supernova remnant

, 1984
Yutaka Matsui, Knox S. Long, J. R. Dickel, E. W. Greisen   +3 more
openalex   +1 more source

Origin of reconnecting current sheets in shocked turbulent plasma. [PDF]

Sci Adv
Wang S, Lu S, Lu Q, Wang R, Ren J, Gao X, Guo J.   +6 more
europepmc   +1 more source

Identification and Characterization of Innate Immunity in Actinidia melanandra in Response to Pseudomonas syringae pv. actinidiae. [PDF]

Plant Cell Environ
Hemara LM, Chatterjee A, Yeh SM, Chen RKY, Hilario E, Lievre LL, Crowhurst RN, Bohne D, Arshed S, Patterson HR, Barrett-Manako K, Thomson S, Allan AC, Brendolise C, Chagné D, Templeton MD, Tahir J, Jayaraman J.   +17 more
europepmc   +1 more source

Predictions for neutrinos and new physics from forward heavy hadron production at the LHC. [PDF]

Eur Phys J C Part Fields
Buonocore L, Kling F, Rottoli L, Sominka J.   +3 more
europepmc   +1 more source

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Supernova Remnant

2014
T. Montmerle
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Supernovae and Their Remnants [PDF]

, 1987
Supernovae (SNe) and supernova remnants (SNRs) represent an important area of research in astrophysics because they are central to our understanding of such diverse fields as the late stages of stellar evolution, mass loss from late-type stars, nucleosynthesis, and interstellar medium processes and abundances. In addition, they provide a laboratory for
Nino Panagia, William P. Blair
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Supernovae and supernova remnants [PDF]

, 2001
A supernova explosion is among the most dramatic events that can be seen. The term ‘supernova’ is somewhat misleading, as such an event represents not a new star (that is, a ‘nova’), but instead the end of a star’s life. Nuclear fusion, the energy source of the stars, creates heavier elements from lighter elements.
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