COMPARING [C ∥], H i, and CO DYNAMICS of NEARBY GALAXIES
Accepted version
Peer-reviewed
Repository URI
Repository DOI
Change log
Authors
Abstract
The HI and CO components of the interstellar medium (ISM) are usually used to
derive the dynamical mass M_dyn of nearby galaxies. Both components become too
faint to be used as a tracer in observations of high-redshift galaxies. In
those cases, the 158
Description
Keywords
Journal Title
Conference Name
Journal ISSN
1538-3881