Protoplanetary Nebulae

Protoplanetary Nebulae is a short-lived transitional phase in stellar evolution, classified as a circumstellar nebula, that forms when an asymptotic giant branch star expels its outer layers, which are subsequently ionized by the increasing ultraviolet radiation from the hot central remnant, distinguishing it from planetary nebulae by its cooler central star and dominant infrared emission from dust.

979

Publications

54K

Citations

2.1K

Authors

673

Institutions

Publications per year

2017–2026

75

Variants

Pre-planetary Nebulae

Authors

2.1K

  1. SK
    Sun Kwok

    University of Calgary, Canada

    46 publications · 2.9K citations

    34

    h-index

  2. BJ
    Bruce J. Hrivnak

    Valparaiso University, United States

    34 publications · 1.8K citations

    27

    h-index

  3. RS
    R. Sahai

    Jet Propulsion Laboratory, United States

    34 publications · 2.2K citations

    26

    h-index

  4. VB
    V. Bujarrabal

    Spanish National Observatory, Spain

    24 publications · 1.2K citations

    19

    h-index

  5. AA
    A. A. Zijlstra

    University of Manchester, United Kingdom

    23 publications · 900 citations

    19

    h-index

1–5 of 2.1K

Venues

  1. The Astrophysical Journal

    ApJ · 414 publications · 24.5K citations

    78

    h-index

  2. Astronomy and Astrophysics

    102 publications · 4.3K citations

    39

    h-index

  3. The Astronomical Journal

    AJ · 62 publications · 4.3K citations

    38

    h-index

  4. Monthly Notices of the Royal Astronomical Society

    115 publications · 4.4K citations

    37

    h-index

  5. Icarus

    27 publications · 4.1K citations

    23

    h-index

1–5