Results 81 to 90 of about 1,779 (176)
Astrochemistry and Observations [PDF]
8 pages, 6 figures in text, From Fourth Cologne-Bonn-Zermatt-Symposium, The Dense Interstellar Matter in ...
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Summary: Early Earth’s UV-rich environment, together with abundant transition metals, likely shaped the stability of biomolecules. We investigated how cations influence the UV (254 nm) stability of diphenylalanine (FF).
Wei Tang +8 more
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Infrared spectroscopic observations have established the presence of solid methanol (CH _3 OH) in the interstellar medium and in solar system ices, but the abundance of frozen CH _3 OH cannot be deduced without accurate band strengths, optical constants,
Reggie L. Hudson +2 more
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The infrared (IR) band strengths most often used to quantify laboratory and astronomical spectra of CO _2 ices are now 60 yr old, from a time of slide rules and vacuum-tube technology.
Reggie L. Hudson +2 more
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The black marl of the Fish Clay at Højerup is mainly made up of biogenic calcite and cheto-Mg-smectite. We suggest that the formation of the smectite occurred during the latest Maastrichtian (or earlier) and that it represents a short period of rapid ...
P.I. PREMOVIC +2 more
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Computational Astrochemistry Journey towards the molecular universe
In astrochemistry, computational methods play a crucial role in addressing fundamental astronomical questions. Interstellar molecules profoundly influence the chemistry and physics of the interstellar medium (ISM), playing pivotal roles in planet formation and the emergence of life. Understanding their chemistry relies on theoretical approaches such as
Campisi, D., Perrero, J., Balucani, N.
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The Seasons of a Career in Physical Chemistry: Olivia Harper Wilkins. [PDF]
Wilkins OH +3 more
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Optical Anisotropy as a Probe of Proton Ordering at Ice Surfaces. [PDF]
Muroni A +4 more
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