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Autor:
Blok, WJGD, Walter, F, Smith, JDT, Herrera-Camus, R, Bolatto, AD, Requena-Torres, MA, Crocker, AF, Croxall, KV, Kennicutt, RC, Koda, J, Armus, L, Boquien, M, Dale, D, Kreckel, K, Meidt, S
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 1
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ea8da96324e10f2f0e9d55a38a9a294c
https://www.repository.cam.ac.uk/handle/1810/256261
https://www.repository.cam.ac.uk/handle/1810/256261
