Results 1 to 10 of about 1,920,958 (265)
On determination of the cosmic ray flux using molecular hydrogen absorption lines [PDF]
We outline a procedure for estimating the cosmic ray flux at remote locations where molecular hydrogen absorption lines have been detected. The method relies on several assumptions whose validity in the local Galactic ISM has been independently verified,
Ćirković Milan M., Damjanov I.
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Polarization Transfer Rates by Isotropic Collisions between Astrophysical SiO Molecule and Electrons
We are interested in quantum calculations of polarization transfer (PT) rates due to collisions of the SiO molecule with the electrons. We determine the inelastic PT rates associated to the transitions: X 1Σ+→3Π; X 1Σ+→3Σ+; X 1Σ+→3Δ; X 1Σ+→3Σ−.
Moncef Derouich +3 more
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Cosmic-Ray Induced Diffusion in Interstellar Ices
Cosmic rays are able to heat interstellar dust grains. This may enhance molecule mobility in icy mantles that have accumulated on the grains in dark cloud cores.
Kalvāns Juris
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The Effect of an Inert Solid Reservoir on Molecular Abundances in Dense Interstellar Clouds
The question, what is the role of freeze-out of chemical species in determining the molecular abundances in the interstellar gas is a matter of debate.
Kalvāns Juris, Shmeld Ivar
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Hydrogen Bonds and Life in the Universe
The scientific community is allocating more and more resources to space missions and astronomical observations dedicated to the search for life beyond Earth.
Giovanni Vladilo, Ali Hassanali
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Alternanthera philoxeroides is an amphibious invasive weed that can colonize both aquatic and terrestrial habitats. Individuals growing in different habitats exhibit extensive phenotypic variation but little genetic differentiation. Little is known about
Lexuan eGao +5 more
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Cold Stress, Freezing Adaptation, Varietal Susceptibility of Olea europaea L.: A Review
Olive (Olea europaea L.) is an evergreen xerophytic tree characterizing vegetative landscape and historical-cultural identity of the Mediterranean Basin.
Raffaella Petruccelli +7 more
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UV irradiation of ethanol-containing interstellar ice analogs
Context. Ethanol (CH3CH2OH) has been detected in interstellar ices within regions associated with the early stages of star and planet formation. Because of its ability to form through multiple gas- and solid-phase pathways, ethanol is found in a range of
DeVine J. A. +5 more
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Chemistry and ro-vibrational excitation of CH+ in the planetary nebula NGC 7027
Context. Small carbon hydride cations, such as methylidynium (CH+), are important in the chemistry of the interstellar medium. They participate in a network of gas-phase reactions with a range of molecular and atomic species and lead to the formation of ...
Sil M. +7 more
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Slow-electron-triggered chemistry in interstellar methanol-water ices
Water and, to a lesser extent, methanol are widespread in interstellar space as ices, where sustained exposure to ionizing radiation promotes the formation of complex compounds such as prebiotic molecules via multi-step reactions.
Abdoul-Carime H., Kopyra J.
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