Molecular Cloud Interfaces
Molecular Cloud Interfaces is a theoretical construct that delineates the transitional zones between H II regions and photodissociation regions, where molecular clouds are subject to intense far-ultraviolet radiation and dynamical feedback, thereby governing the physical and chemical processes that regulate star formation and interstellar medium evolution.
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C + Emission from the Magellanic Clouds. I. The Bright H II Region Complexes N159 and N160
F. P. Israel, P. R. Maloney, N. Geis et al. · The Astrophysical Journal · 1996 · 110 citations
Natural Sciences, Astronomy, Physics +16
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Max Planck Institute for Extraterrestrial Physics
Garching bei München, Germany
4 h-index
9 publications
641 citations

Centre National de la Recherche Scientifique
Paris, France
3 h-index
9 publications
333 citations

University of Cologne
Cologne, Germany
3 h-index
12 publications
548 citations

Cornell University
Ithaca, United States
3 h-index
3 publications
124 citations

University of Manchester
Manchester, United Kingdom
2 h-index
4 publications
110 citations
Astrophysique, Instrumentation et Modélisation
Gif-sur-Yvette, France
2 h-index
8 publications
304 citations
Commissariat à l'Énergie Atomique et aux Énergies Alternatives
Paris, France
2 h-index
8 publications
304 citations
Max Planck Society
Munich, Germany
2 h-index
4 publications
178 citations
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ApJ · 14 publications · 711 citations
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2 publications · 92 citations
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Repository · 2 publications · 80 citations
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2 publications · 55 citations
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1 publications · 19 citations
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