Stellar Outflows

Stellar Outflows is a physical phenomenon characterized by the continuous ejection of matter and energy from a star’s outer layers into the surrounding interstellar medium, distinguished from other mass loss mechanisms by its sustained, often asymmetric, and hydrodynamically driven nature.

664

Publications

45.5K

Citations

1.8K

Authors

599

Institutions

Publications per year

2017–2026

161

Authors

1.8K

  1. JB
    John Bally

    University of Colorado Boulder, United States

    18 publications · 1.7K citations

    18

    h-index

  2. RB
    R. Bachiller

    Spanish National Observatory, Spain

    12 publications · 1K citations

    12

    h-index

  3. RM
    R. Maiolino

    University of Cambridge, United Kingdom

    11 publications · 1.5K citations

    11

    h-index

  4. TP
    T. P. Ray

    Dublin Institute For Advanced Studies, Ireland

    10 publications · 578 citations

    11

    h-index

  5. MT
    M. Tafalla

    Spanish National Observatory, Spain

    10 publications · 570 citations

    10

    h-index

1–5 of 1.8K

Venues

  1. The Astrophysical Journal

    ApJ · 241 publications · 17.6K citations

    74

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    121 publications · 7.4K citations

    46

    h-index

  3. Astronomy and Astrophysics

    84 publications · 4.5K citations

    40

    h-index

  4. The Astronomical Journal

    AJ · 24 publications · 1K citations

    20

    h-index

  5. The Astrophysical Journal Letters

    15 publications · 961 citations

    14

    h-index

1–5