Results 181 to 190 of about 4,494 (233)

The UV Photodissociation Spectrum of FeOH⁺: Electronic Insight into the Simplest Iron Hydroxide Complexes. [PDF]

J Phys Chem A
Jin S, Juanes M, Reimann M, van der Linde C, Ončák M, Beyer MK.   +5 more
europepmc   +1 more source

Interstellar Mapping And Acceleration Probe: The NASA IMAP Mission. [PDF]

Space Sci Rev
McComas DJ, Christian ER, Schwadron NA, Gkioulidou M, Allegrini F, Baker DN, Bzowski M, Clark G, Cohen CMS, Cohen I, Collura C, Cully MJ, Dalla S, Desai MI, Driesman A, Eng D, Fox NJ, Funsten HO, Fuselier SA, Galli A, Giacalone J, Hahn J, Hegarty KP, Horbury T, Horanyi M, Kistler LM, Kubiak MA, Kubota S, Livi S, Lugaz N, Lee CO, Luhmann J, Matthaeus W, Mitchell DG, Mitchell JG, Moebius E, Pope S, Provornikova E, Rankin JS, Reisenfeld DB, Reno C, Richardson JD, Russell CT, Shaw-Lecerf MM, Scherrer J, Skoug RM, Shen MM, Spence HE, Sternovsky Z, Strumik M, Szalay JR, Tapley M, Tokumaru M, Turner DL, Weidner S, Westlake J, Wurz P, Zank GP.   +57 more
europepmc   +1 more source

Hot Sulfur on the Rocks: The Reaction of Electronically Excited Sulfur Atoms with Water in an Ice-Surface Model. [PDF]

ACS Earth Space Chem
Di Genova G, Perrero J, Rosi M, Ceccarelli C, Rimola A, Balucani N.   +5 more
europepmc   +1 more source

Ionic Reactant Orientation Inhibits Ion-Neutral Reactions at Low Temperatures. [PDF]

JACS Au
Peng Y, Li J, Song Z, Li M, Xiao Y, Wang X, Wang T, Xie Y, Li J, Yang T.   +9 more
europepmc   +1 more source

Revealing SO₂ and CO₂ adsorption features on forsterite <i>via</i> IR spectroscopy and automated computational approaches.

Phys Chem Chem Phys
Mates-Torres E, Escolano Casado G, Mino L, Balucani N, Ugliengo P, Rimola A.   +5 more
europepmc   +1 more source

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Interstellar Dust Clouds

Nature, 1971
THE failure, thus far, to detect gaseous emission lines from circumstellar dust clouds1–3 and from Bok globules2 raises the possibility that such clouds consist solely of dust grains. The possibility has previously been largely discounted on the grounds that relative diffusion of the grains and gas is slow and inefficient requiring time scales which ...
openaire   +2 more sources

Interstellar Molecular Clouds

Science, 1986
The interstellar medium in our galaxy contains matter in a variety of states ranging from hot plasma to cold and dusty molecular gas. The molecular phase consists of giant clouds, which are the largest gravitationally bound objects in the galaxy, the primary reservoir of material for the ongoing birth of new stars, and the medium regulating the ...
openaire   +2 more sources

Interstellar Molecules and Dense Clouds

Science, 1971
Current knowledge of the interstellar medium is discussed on the basis of recent published studies. The subjects considered include optical identification of interstellar molecules, radio molecular lines, interstellar clouds, isotopic abundances, formation and disappearance of interstellar molecules, and interstellar probing techniques.
D M, Rank, C H, Townes, W J, Welch
openaire   +2 more sources