Results 241 to 250 of about 10,661 (258)

ASTROCHEMISTRY: AN UNFINISHED SYMPHONY

Proceedings of the Dalgarno Celebratory Symposium, 2009
Alex Dalgarno has introduced many of the themes that define current research in astrochemistry. Variations on these themes will continue to be played out well into the future. Clear and unambiguous tests of theories of formation of interstellar molecules remain elusive; however, the understanding of fluorine chemistry appears to offer one success story.
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Rotational spectroscopy and astrochemistry

Journal of Molecular Structure, 1995
Abstract During the last 25 years, the close collaboration between laboratory spectrocopists and astrophysicists allowed the detection of about one hundred different molecular species in the interstellar medium, largely via their rotational emission spectra.
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Interstellar Carbonaceous Dust and Its Formation Pathways: From an Experimental Astrochemistry Perspective

Journal of the Indian Institute of Science, 2023
Arijit Roy, V. Surendra, R. Ramachandran, J. Meka, Supryia Gupta, P. Janardhan, B. N. Rajasekhar, H. Hill, Anil Bhardwaj, N. Mason, B. Sivaraman   +10 more
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Suprathermal particles in astrochemistry

Russian Chemical Reviews, 2019
The kinetic Monte Carlo method, used in astrochemistry to investigate suprathermal (hot) particles at the molecular level, is presented. Different modifications of this method, aimed at studying the influence of suprathermal particles in the processes occurring ...
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The 1.5 μm Band of Cyanoacetylene as a Spectroscopic Target in Astrochemistry.

Journal of Physical Chemistry Letters
The search for prebiotic molecules officially entered a new era with the launch of the James Webb Space Telescope. The capabilities of the near-infrared instrumentation on board offer greater sensitivity and resolution than have ever been available in a ...
Thomas Howard, Sanjana Maheshwari, Grace J Yeh, Shannon E Ganley, Leah G Dodson   +4 more
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Current Views on Astrochemistry

1987
Astrochemistry is the study of the formation and destruction of interstellar and circumstellar molecules. Such molecules have been a major field of astrophysical investigation for about 17 years. As of 1987 January, 66 species are identified, and the discovery rate is about three per year.
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Introduction: Astrochemistry

Chemical Reviews, 2013
Eric, Herbst, John T, Yates
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Recent developments in astrochemistry

AIP Conference Proceedings, 1994
I describe the astronomical regions in which chemistry is known to occur, and list the types of molecules that have been positively identified. Some of the successes and failures of chemistries that have been proposed to give rise to these molecular species are reviewed.
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Interstellar Molecules and Astrochemistry

1988
The quantitative study of the interstellar medium (ISM) began with Hartman’s detection in 1904 of the resonance lines of Ca and K, seen in absorption against bright stars by intervening diffuse clouds. Other atoms (Na,Fe,Ti) were subsequently detected, although the overwhelming abundance of H was not recognized until the 1930s.
Lucy M. Ziurys, Barry E. Turner
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Computational astrochemistry: general discussion.

Faraday discussions, 2023
Stefan T. Bromley, S. Brünken, C. Ceccarelli, M. Cordiner, Kristen Darnell, Gwenaëlle Dufour, Athena Flint, R. Garrod, M. Gudipati, Joshua Halpern, Eric Herbst, Ko-Yun Huang, Inga Kamp, N. Madhusudhan, M. McCoustra, A. Suits, Marie Van de Sande, E. V. van Dishoeck, S. Viti, Laurent Wiesenfeld   +19 more
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