Zobrazeno 1 - 10
of 4 292
pro vyhledávání: '"Interstellar cloud"'
Autor:
Itzhak Goldman
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 504:4493-4496
The observational structure function of the scintillations of the radio pulsar PSR B0950+08, was fitted, a decade ago, with a power law with index $1 \pm 0.01$. This was interpreted as an {\em appreciable deviation} from the, commonly observed index
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 503:3522-3539
Interstellar clouds can act as target material for hadronic cosmic rays; gamma rays subsequently produced through inelastic proton-proton collisions and spatially associated with such clouds can provide a key indicator of efficient particle accelerat
Autor:
V. Kofman, K.-J. Chuang, E. F. van Dishoeck, A. R. Clements, Gleb Fedoseev, Harold Linnartz, Robin T. Garrod, Mi Wha Jin, Herma M. Cuppen, Sergio Ioppolo, D. Qasim
Publikováno v:
Nature Astronomy, 5, 197-205
Nat. Astron.
Nature Astronomy
Nature Astronomy, 5, pp. 197-205
Nat. Astron.
Nature Astronomy
Nature Astronomy, 5, pp. 197-205
The detection of the amino acid glycine and its amine precursor methylamine on the comet 67P/Churyumov-Gerasimenko by the Rosetta mission provides strong evidence for a cosmic origin of prebiotics on Earth. How and when such complex organic molecules
Autor:
T.V. Salnikova, S. Ya. Stepanov
Publikováno v:
Computational Mathematics and Mathematical Physics. 60:1730-1736
A mathematical model of the early stage of the formation of interstellar clouds resulting from the interaction of oppositely directed cosmic particle flows and evolution of the clouds into planetary systems is proposed. An important role in the evolu
Publikováno v:
Mathematical Physics and Computer Simulation. :41-56
It is believed that the taxonomy of interstellar clouds in their vicinity can serve as an indicator of the features of the geometry and intensity of galactic shock waves. In this paper, the authors present the results of a detailed two-dimensional hy
Publikováno v:
Chemical Reviews. 120:4616-4659
Despite the generally hostile nature of the environments involved, chemistry does occur in space. Molecules are seen in environments that span a wide range of physical and chemical conditions and that clearly were created by a multitude of chemical p
Autor:
Shmuel Bialy
Publikováno v:
Communications Physics, Vol 3, Iss 1, Pp 1-7 (2020)
Low energy cosmic-rays (CRs) are responsible for gas heating and ionization of interstellar clouds, which in turn introduces coupling to Galactic magnetic fields. So far the CR ionization rate (CRIR) has been estimated using indirect methods, such as
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 491:4325-4333
Blue-shifted Broad Absorption Lines (BALs) detected in quasar's spectra are indicative of AGN outflows. We show, using 2D hydrodynamical simulations, that disruption of interstellar clouds by a fast AGN wind can lead to formation of cold, dense high
Autor:
Abdelilah Benallou
Publikováno v:
Journal of Taibah University for Science, Vol 13, Iss 1, Pp 105-111 (2019)
The mechanism formation of adenine is determinate in the gas phase, by using density functional theory (DFT) method at the B3LYP hybrid together with 6-311g(d,p) basis set level. Thus, we have investigated the structures and mechanisms pathway as wel
In this contribution we present the first numerical simulations of a relativistic outflow propagating through the inner hundreds of parsecs of its host galaxy, including atomic and ionised hydrogen, and the cooling effects of ionisation. Our results
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0c7c978c8aff1e0ff8ffd993cbe5ab8f
http://arxiv.org/abs/2109.15234
http://arxiv.org/abs/2109.15234