Gas and dust cooling along the major axis of M 33 (HerM33es). Herschel/PACS [C II] and [O I] observations
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. Aims: We investigate the relationship between the two major gas cooling lines and the total infrared (TIR) dust continuum. Methods: We mapped
Kramer, Carsten et al.
Fecha de publicación:
7
2020