Results 51 to 60 of about 4,701,578 (85)
The hydrodynamics of a supernova shock in the interstellar medium
, 2004 The interactions of a supernova blast wave with the inhomogeneities of the interstellar medium have been observed both in the young supernova remnants, with ages ∼ 102 yr, and in the middle-aged supernova remnants older than ∼ 104 yr. Low mass supernovae
R. Bedogni
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Cross-NASA divisional relevance of an Ice Giant mission. [PDF]
Philos Trans A Math Phys Eng Sci, 2020 Cohen IJ, Rymer AM.
europepmc +1 more source
Studying The Local Interstellar Medium through Measurements of Interstellar Hydrogen Inside the Heliosphere [PDF]
, 2020 The Interstellar Medium (ISM) incorporates all the matter that fills up the space between the stars of a galaxy. Interstellar matter consists mainly of hydrogen and helium gas, either in atomic or ionized form, as well as some heavier atoms, molecules ...
Wikberg, Frida
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Particle Production in the Interstellar Medium
, 1996 The flux of neutrinos and photons originating from cosmic ray interactions with the interstellar medium in the galaxy is calculated based on current models for high energy particle interactions.
Thunman, Mats, Ingelman, Gunnar,
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, 2013 Neutral hydrogen atoms that travel into the heliosphere from the local interstellar medium (LISM) experience strong effects due to charge exchange and radiation pressure from resonant absorption and re-emission of Lyα.
French, J. +13 more
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, 1978 Observations of the spectral lines of a great many interstellar molecules has made it possible for radio astronomers to construct a scenario for the formation of ...
Knapp, Gillian
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Physical structure of the local interstellar medium
, 2020 The physical structure and morphology of the interstellar medium that surrounds our solar system directly effects the heliosphere and the interplanetary environment.
S Redfield, B E Wood, J L Linsky
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Mrs. Marie O\u27Neal wipes her brow as she pretends to pump air into the American Airlines Astrosphere at Seminary South. Fort Worth Star-Telegram Morning May 24, 1967.https://mavmatrix.uta.edu/specialcollections_startelegram1960s/5720/thumbnail ...
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A dense gas survey of the gamma-ray sources HESS J1731-347 and HESS J1729-345
, 2014 The results of Mopra molecular spectral line observations towards the supernova remnant HESS J1731−347 (G353.6−0.7) and the unidentified gamma-ray source HESS J1729−345 are presented.
Maxted, Nigel I. (R19203) +10 more
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Astrospheres and Solar-like Stellar Winds. [PDF]
Living Rev Sol Phys, 2004 Wood BE.
europepmc +1 more source