High Mass Star Formation : A Review
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Pre-published on:
May 06, 2019
Published on:
November 20, 2019
Abstract
This review gives the state-of-art knowledge of high mass star formation gained from observa- tional surveys from millimeter to near-infrared wavelengths. In particular a giant molecular cloud (NGC 6334) is taken as an example of a study of high mass star formation regions including Herschel, Spitzer and near-infrared data.
DOI: https://doi.org/10.22323/1.331.0029
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Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.
Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.