Article ISI SCOPUS
Astrophysical Journal  (2019)

Using [CII] 158 mu m Emission from Isolated ISM Phases as a Star Formation Rate Indicator

Sutter J.; Dale, D. A.; Pelligrini E.W.; Smith, J D T; Bolatto, A. D.; Crocker A.; Draine, B.; Hunt, L. K.; Roussel H.; Wolfire, M. G.

Abstract

The brightest observed emission line in many star-forming galaxies is the ?m line, making it detectable up to z;?;7. In order to better understand and quantify the

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Título según WOS: Using [CII] 158 mu m Emission from Isolated ISM Phases as a Star Formation Rate Indicator
Título según SCOPUS: Using [C II] 158 ?m Emission from isolated ism phases as a star formation rate indicator
Título de la Revista: Astrophysical Journal
Volumen: 886
Número: 1
Editorial: Institute of Physics Publishing
Fecha de publicación: 2019
Idioma: English
DOI:

10.3847/1538-4357/ab4da5
Notas: ISI, SCOPUS