Publication Date:
2003-12-13
Description:
Detailed laboratory experiments on the formation of HD from atom recombination on amorphous solid water films show that this process is extremely efficient in a temperature range of 8 to 20 kelvin, temperatures relevant for H2 formation on dust grain surfaces in the interstellar medium (ISM). The fate of the 4.5 electron volt recombination energy is highly dependent on film morphology. These results suggest that grain morphology, rather than the detailed chemical nature of the grain surface, is most important in determining the energy content of the H2 as it is released from the grain into the ISM.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Hornekaer, L -- Baurichter, A -- Petrunin, V V -- Field, D -- Luntz, A C -- New York, N.Y. -- Science. 2003 Dec 12;302(5652):1943-6.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Department of Physics, University of Southern Denmark, Denmark. hornekaer@fysik.sdu.dk〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/14671297" target="_blank"〉PubMed〈/a〉
Keywords:
Astronomical Phenomena
;
*Astronomy
;
*Cosmic Dust
;
Extraterrestrial Environment
;
Hydrogen/*chemistry
;
Spectrum Analysis
;
Temperature
;
Thermodynamics
;
Water
Print ISSN:
0036-8075
Electronic ISSN:
1095-9203
Topics:
Biology
,
Chemistry and Pharmacology
,
Computer Science
,
Medicine
,
Natural Sciences in General
,
Physics
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