Constraining the magnetohydrodynamic turbulence around Geminga by observing the γ-ray halo beyond 100 TeV. [PDF]
Tibet ASγ Collaboration.
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Multi-messenger gravitational lensing. [PDF]
Smith GP +40 more
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Information-Entropy Analysis of Stellar Evolutionary Stages with Application to FS CMa Objects. [PDF]
Zhanabaev Z, Akniyazova A, Ashimov Y.
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Evolution of Supernova Remnants. I. Interacting Supernova Remnants
application ...
openaire
Assembling genomes of non-model plants: A case study with evolutionary insights from Ranunculus (Ranunculaceae). [PDF]
Karbstein K +15 more
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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 ...
openaire
Quantum sensing for NASA science missions. [PDF]
Mercer CR +6 more
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A connection between proto-neutron-star Tayler-Spruit dynamos and low-field magnetars. [PDF]
Igoshev A +5 more
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60Fe deposition during the late Pleistocene and the Holocene echoes past supernova activity. [PDF]
Wallner A +13 more
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False positives in gravitational wave campaigns: the electromagnetic perspective. [PDF]
Oates S.
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