TY  - JOUR 
AU  - Kramer, Carsten
AU  - Verley, Simon
PY  - 2020
UR  - http://hdl.handle.net/10481/63671
AB  - 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...
LA  - eng
PB  - EDP Sciences
KW  - Galaxies: ISM
KW  - Galaxies: individual:M33
KW  - Infrared: galaxies
KW  - Infrared: ISM
TI  - Gas and dust cooling along the major axis of M 33 (HerM33es) Herschel/PACS [C ii] and [O i] observations
DO  - 10.1051/0004-6361/201936754
ER  -