Results 71 to 80 of about 921 (183)
Mapping the Dense Molecular Gas toward 13 Supernova Remnants
Supernova remnants (SNRs) can exert strong influence on molecular clouds (MCs) through interaction by shock wave and cosmic rays. In this paper, we present our mapping observation of HCO ^+ and $\mathrm{HCN}$ 1–0 lines toward 13 SNRs interacting with MCs,
Tian-Yu Tu, Yang Chen, Qian-Cheng Liu
doaj +1 more source
Nonthermal Signatures of Radiative Supernova Remnants
The end of supernova remnant (SNR) evolution is characterized by a so-called “radiative” stage, in which efficient cooling of the hot bubble inside the forward shock slows expansion, leading to eventual shock breakup.
Rebecca Diesing +4 more
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Supernova Remnants with Fermi Large Area Telescope
The Large Area Telescope (LAT), on-board the Fermi satellite, proved to be, after 8 years of data taking, an excellent instrument to detect and observe Supernova Remnants (SNRs) in a range of energies running from few hundred MeV up to few hundred GeV ...
Caragiulo M., Di Venere L.
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Supernova blast wave shock is a very important site of cosmic-ray acceleration. However, the detailed physical process of acceleration, in particular, nonlinear interplay between cosmic-ray streaming and magnetic field amplification, has not been studied
Tsuyoshi Inoue +2 more
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Deep Optical Emission-line Images of Nine Known and Three New Galactic Supernova Remnants
Deep optical emission-line images are presented for nine known plus three new Galactic supernova remnants (SNRs), all but one having at least one angular dimension >1°.
Robert A. Fesen +16 more
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Supernova remnants (SNRs) exhibit varying degrees of anisotropy, which have been extensively modeled using numerical methods. We implement a technique to measure anisotropies in SNRs by calculating power spectra from their high-resolution images. To test
Soham Mandal +3 more
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Supernovae and the Arrow of Time. [PDF]
Abarzhi SI +4 more
europepmc +1 more source
The maximum energy of electrons in supernova remnant (SNR) shocks is typically limited by radiative losses, where the synchrotron cooling time equals the acceleration time.
Vincenzo Sapienza +7 more
doaj +1 more source
Continuous solutions of cosmic-rays and waves in astrophysical environments. [PDF]
Irshad K +5 more
europepmc +1 more source
A persistent influence of supernovae on biodiversity over the Phanerozoic. [PDF]
Svensmark H.
europepmc +1 more source

