Results 81 to 90 of about 3,453 (176)

Chemical Simulations of Cyanomethanimine in Interstellar Medium

, 2017
Simulating chemical reactions that involve the creation and destruction of cyanomethanimine is critical in the understanding of chemistry in interstellar medium.
Webb, Matthew T
core  

On the Abundances of Interstellar Molecules

The Astrophysical Journal, 1972
W. D. Watson, E. E. Salpeter
openaire   +1 more source

Synthesis of Molecules in Interstellar Clouds & Star Formation [PDF]

, 1981
237-240Study of the formation and destruction processes of interstellar molecules may throw certain light on interstellar medium. Formation and destruction processes of some interstellar molecules are proposed on the basis of laboratory data.
Ghosh, K K, Ghosh, S N
core  

The Abundance of Interstellar Carbon

The Astrophysical Journal, 1996
Jason A. Cardelli, David M. Meyer, M. Jura, Blair D. Savage   +3 more
openaire   +1 more source

On the Abundance of Interstellar OH

The Astrophysical Journal, 1966
T. O. Carroll, E. E. Salpeter
openaire   +1 more source

Direct Samples of Interstellar and Interplanetary Material with IMAP. [PDF]

Space Sci Rev
Szalay JR, Provornikova E, Ayari E, Bzowski M, Christian ER, Funsten HO, Galli A, Gkioulidou M, Horányi M, Livi S, McComas DJ, Möbius E, Ogasawara K, Rahmanifard F, Rankin JS, Reisenfeld DB, Schwadron NA, Sternovsky Z, Swaczyna P, Turner D, Zank GP, Zirnstein EJ.   +21 more
europepmc   +1 more source

A new search for interstellar C3

, 1988
A new, very sensitive search for interstellar triatomic carbon has resulted in upper limits for a few diffuse clouds of order 1010 cm – 2, or about 10 – 11 with respect to hydrogen.
Joseph, Charles L, Snow, Theodore P, Seab, C Gregory   +2 more
core  

Non-equilibrium preparation of (<i>E</i>)-phosphinimine (HPNH, X¹A') - a precursor to prebiotic phosphorylating agents. [PDF]

Chem Sci
Wang J, Sun BJ, Bergantini A, Wang Z, McAnally M, Marks JH, Chang AHH, Eckhardt AK, Kaiser RI.   +8 more
europepmc   +1 more source

THE SENSITIVITY OF GAS-PHASE CHEMICAL MODELS OF INTERSTELLAR CLOUDS TO C AND O ELEMENTAL ABUNDANCES AND TO A NEW FORMATION MECHANISM FOR AMMONIA

, 1997
The e†ects of variations in the gas-phase carbon-to-oxygen elemental abundance ratio (0.42 C/O 1.2) and the absolute gas-phase carbon and oxygen elemental abundances on calculated molecu-lar concentrations have been studied for three gas-phase chemical ...
Eric Herbst, R. Terzieva
core  

Atom Addition Formation of Thionylimide (HNSO) on Interstellar Dust Grains: Chemical Routes Requiring Oxygen and Nitrogen Atom Surface Diffusion. [PDF]

ACS Earth Space Chem
Del Valle JC, Sanz-Novo M, Kästner J, Furuya K, Rivilla VM, Martín-Doménech R, Molpeceres G.   +6 more
europepmc   +1 more source