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.

25

Publications

1.1K

Citations

91

Authors

58

Institutions

Publications per year

2017–2026

4

Authors

91

  1. GJ
    G. J. Stacey

    Cornell University, United States

    3 publications · 376 citations

    3

    h-index

  2. JS
    J. Stützki

    University of Cologne, Germany

    2 publications · 96 citations

    2

    h-index

  3. NG
    N. Geis

    Max Planck Institute for Extraterrestrial Physics, Germany

    2 publications · 181 citations

    2

    h-index

  4. RG
    R. Genzel

    Max Planck Institute for Extraterrestrial Physics, Germany

    2 publications · 259 citations

    2

    h-index

  5. AI
    A. I. Harris

    University of Maryland, College Park, United States

    2 publications · 259 citations

    2

    h-index

1–5 of 91

Venues

  1. The Astrophysical Journal

    ApJ · 14 publications · 711 citations

    12

    h-index

  2. Astronomy and Astrophysics

    2 publications · 92 citations

    2

    h-index

  3. Springer Link (Chiba Institute of Technology)

    Repository · 2 publications · 80 citations

    2

    h-index

  4. 2

    h-index

  5. Meteoritics and Planetary Science

    1 publications · 19 citations

    1

    h-index

1–5