Results 121 to 130 of about 1,520 (178)

Transport of Electrons in Tangled Magnetic Fields. [PDF]

Space Sci Rev
Verscharen D, Jeffrey N, Artemyev A, Coburn JT, Kunz MW, Pezzi O, Riquelme M, Svenningsson I, Wilson Iii LB.   +8 more
europepmc   +1 more source

Experimental VUV Photoionization of C₇₀ and Vibrationally Resolved Spectra of the Excited Electronic States of the C₇₀ ^<b>+</b> Cation. [PDF]

ACS Earth Space Chem
Ganner L, Garcia GA, Schwell M, Kappe M, Nahon L, Gruber E, Hrodmarsson HR.   +6 more
europepmc   +1 more source

Defects at play: Shaping the photophysics and photochemistry of ice. [PDF]

Proc Natl Acad Sci U S A
Monti M, Jin Y, Mirón GD, Kundu A, Govoni M, Galli G, Hassanali A.   +6 more
europepmc   +1 more source

Ionic Liquid Biospheres. [PDF]

Life (Basel)
Seager S, Bains W, Iakubivskyi I, Agrawal R, Jenkins J, Shinde P, Petkowski JJ.   +6 more
europepmc   +1 more source

Predicting accurate binding energies and vibrational spectroscopic features of interstellar icy species. A quantum mechanical study.

Phys Chem Chem Phys
Bulik A, Martínez-Bachs B, Bancone N, Mates-Torres E, Corno M, Ugliengo P, Rimola A.   +6 more
europepmc   +1 more source

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Local interstellar matter and interstellar bubbles

Astronomical and Astrophysical Transactions, 1992
Abstract Giant bubbles in nearby galaxies and our Galaxy are observed in optics, radio, and X-rays and have different sizes and origins. The largest ones inside the region occupied by the spiral structure have diameters less than 300-400 pc. The Cygnus Superbubble is not an entity, but represent a result of projection of many sources onto the sky.
exaly   +2 more sources

Interstellar Matter and Chemical Evolution

Science, 1984
The determination of chemical abundances of the interstellar medium is related to three different areas of astronomy: pregalactic conditions, stellar evolution, and chemical evolution of galaxies. The observed abundances permit the testing of theories associated with these areas.
M Peimbert, S Torres-Peimbert
exaly   +3 more sources

Topics in Interstellar Matter

Astrophysics and Space Science Library, 1977
exaly   +2 more sources

DETECTION OF ORGANIC MATTER IN INTERSTELLAR GRAINS

Origins of life and evolution of the biosphere, 1997
Star formation and the subsequent evolution of planetary systems occurs in dense molecular clouds, which are comprised, in part, of interstellar dust grains gathered from the diffuse interstellar medium (DISM). Radio observations of the interstellar medium reveal the presence of organic molecules in the gas phase and infrared observational studies ...
openaire   +2 more sources