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Introduction to Astrochemistry
2003At first sight, the interstellar medium presents a very hostile environment to the formation and survival of complex molecules. As we have seen, it is crisscrossed by violent shocks and pervaded by intense UV and X-ray radiation fields, which can easily tear apart delicate molecular bonds.
Michael A. Dopita, Ralph S. Sutherland
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Observational astrochemistry: Recent results
Advances in Space Research, 1989More than 80 molecular species have now been observed by astronomers in the dense interstellar clouds where stars and planets form or in the envelopes expelled by evolved stars. Elemental constituents of these compounds include all of the "biogenic" elements, hydrogen, carbon, nitrogen, oxygen, sulfur, and (most recently) phosphorus.
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?????????????????? ??? 120 ?????? ???? ???????????????????? (Astrochemistry)
2023?????????????????? ?????????????????? 3???7 ?????????????? 1985 ??. ?? ??. ??????, ??????????
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Recent advances in astronomy showed that a variety of simple and complex organic molecules are abundantly observed in the interstellar medium. Astrochemical models confirmed that the physical and chemical conditions in regions where stars and planets are born affect the formation and destruction of life-related molecules in space.
Ioppolo, S.; id_orcid 0000-0002-2271-1781 +7 more
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Ioppolo, S.; id_orcid 0000-0002-2271-1781 +7 more
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LIDA: The Leiden Ice Database for Astrochemistry
Astronomy and Astrophysics, 2022Marina G Rachid +2 more
exaly
VIZSLA—Versatile Ice Zigzag Sublimation Setup for Laboratory Astrochemistry Available to Purchase
Review of Scientific Instruments, 2021Gyorgy Tarczay +2 more
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FAUST VI. VLA1623−2417 B: a new laboratory for astrochemistry around protostars on 50 au scale
Monthly Notices of the Royal Astronomical Society, 2022François Dulieu +2 more
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