Results 161 to 170 of about 34,658 (198)

Photochemical Haze Formation on Titan and Uranus: A Comparative Review. [PDF]

Int J Mol Sci
Dubois D.
europepmc   +1 more source

Navigating Chemical Space through Isomerization Networks and Intermolecular Encounters of Seven Five-Atom Organic Species. [PDF]

ACS Phys Chem Au
Zhang D, Kishimoto N.
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Instantaneous formation of interstellar minerals and mineral quantum dots. [PDF]

RSC Adv
Roy A, Singh SV, Ramachandran R, Meka JK, Ambresh M, Vijay T, Janardhan P, Jayaram V, Venkatraman V, Das A, Hill H, Bhardwaj A, Mason NJ, Sivaraman B.   +13 more
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Flux equipartition in astrophysical plasma turbulence. [PDF]

Sci Adv
Marino R, Xie JH.
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History of individual presolar SiC grains revealed by stellar winds. [PDF]

Nat Commun
Bajo KI, Izumi T, Otsuki Y, Amari S, Yurimoto H.   +4 more
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Gas-phase synthesis of anthracene and phenanthrene via radical-radical reaction induced ring expansions. [PDF]

Sci Adv
Goettl SJ, Turner AM, Krasnoukhov VS, Azyazov VN, Kanayama K, Hemberger P, Mebel AM, Kaiser RI.   +7 more
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Theoretical Studies of Non-Metal Endohedral Fullerenes. [PDF]

Nanomaterials (Basel)
Slanina Z, Uhlík F, Akasaka T, Lu X, Adamowicz L.   +4 more
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Interstellar formation of lactaldehyde, a key intermediate in the methylglyoxal pathway. [PDF]

Nat Commun
Wang J, Zhang C, Marks JH, Evseev MM, Kuznetsov OV, Antonov IO, Kaiser RI.   +6 more
europepmc   +1 more source

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Observations of Small-Scale Interstellar Structure in Dense Atomic Gas

The Astrophysical Journal, 1999
We present high-resolution (R ~ 170,000) Kitt Peak National Observatory coude feed telescope observations of the interstellar K I λ7698 line toward five multiple star systems with saturated Na I components. We compare the K I absorption-line profiles in each of the two (or three) lines of sight in these systems and find significant differences between ...
J. T. Lauroesch, David M. Meyer
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Evidence for the Heating of Atomic Interstellar Gas by Polycyclic Aromatic Hydrocarbons

The Astrophysical Journal, 2001
We report a strong correlation between the [C II] 158 ?m cooling line and the mid-infrared flux in the 5-10 ?m range in a wide variety of star-forming galaxies. The mid-infrared flux is dominated by the aromatic features in emission (AFEs), which are thought to arise from large polycyclic aromatic hydrocarbons (PAHs) and are generally associated with ...
George Helou, Sangeeta Malhotra, David J. Hollenbach, Daniel A. Dale, Alessandra Contursi   +4 more
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