Results 181 to 190 of about 13,144 (210)

A probable Keplerian disk feeding an optically revealed massive young star. [PDF]

Nature
McLeod AF, Klaassen PD, Reiter M, Henshaw J, Kuiper R, Ginsburg A.   +5 more
europepmc   +1 more source

Low-Temperature Aqueous Alteration of Chondrites. [PDF]

Space Sci Rev
Lee MR, Alexander CMO, Bischoff A, Brearley AJ, Dobrică E, Fujiya W, Le Guillou C, King AJ, van Kooten E, Krot AN, Leitner J, Marrocchi Y, Patzek M, Petaev MI, Piani L, Pravdivtseva O, Remusat L, Telus M, Tsuchiyama A, Vacher LG.   +19 more
europepmc   +1 more source

Exo-Geoscience Perspectives Beyond Habitability. [PDF]

Space Sci Rev
Spohn T, Roberge A, Way MJ, Duarte JC, Miozzi F, Baumeister P, Byrne P, Lineweaver CH.   +7 more
europepmc   +1 more source

Fundamental Role of N-O Bond-Containing Compounds in Prebiotic Synthesis. [PDF]

JACS Au
Sukhorukov AY.
europepmc   +1 more source

Relationship between ices and gas phase organic compounds in simulated extraterrestrial environments. [PDF]

Commun Chem
Javelle T, Duvernay F, Ruf A, Granjon C, Selliez L, Danger G.   +5 more
europepmc   +1 more source

Optical properties of circumstellar and cometary grains

, 2005
openaire   +1 more source

Physicochemical Controls on the Compositions of the Earth and Planets. [PDF]

Space Sci Rev
Sossi PA, Hin RC, Kleine T, Morbidelli A, Nimmo F.   +4 more
europepmc   +1 more source

Abiotic formation of alkylsulfonic acids in interstellar analog ices and implications for their detection on Ryugu. [PDF]

Nat Commun
McAnally M, Bocková J, Herath A, Turner AM, Meinert C, Kaiser RI.   +5 more
europepmc   +1 more source

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The origin of circumstellar silicon carbide grains found in meteorites

Meteoritics, 1995
Abstract— Condensation calculations for C‐rich circumstellar envelopes are used to model the condensation sequence of C, TiC, and SiC, and trace‐element patterns observed in circumstellar SiC grains. Some properties of carbon star envelopes are briefly discussed, and condensation temperatures for major and trace elements are computed for a wide array ...
K Lodders, B Fegley
exaly   +2 more sources