Article ISI
ASTRONOMY & ASTROPHYSICS  (2020)

Gas and dust cooling along the major axis of M 33 (HerM33es) Herschel/PACS [C-II] and [O-I] observations

Nikola, Thomas; Anderl, Sibylle; Bertoldi, Frank; Buchbender, Christof; Combes, Francoise; Israel, Frank; Rollig, Markus; Schuster, Karl; Tabatabaei, Fatemeh; van der Tak, Floris; van der Werf, Paul; Wiedner, Martina; Xilouris, Emmanuel M.

Abstract

Context. M 33 is a gas rich spiral galaxy of the Local Group. Its vicinity allows us to study its interstellar medium (ISM) on linear scales corresponding to the sizes of individual giant molecular clouds.

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Título según WOS: Gas and dust cooling along the major axis of M 33 (HerM33es) Herschel/PACS [C-II] and [O-I] observations
Título de la Revista: ASTRONOMY & ASTROPHYSICS
Volumen: 639
Editorial: EDP SCIENCES S A
Fecha de publicación: 2020
DOI:

10.1051/0004-6361/201936754
Notas: ISI