Probing star formation and ISM properties using galaxy disk inclination: III. Evolution in dust opacity and clumpiness between redshift 0.0 < z < 0.7 constrained from UV to NIR

Author(s):
Giessen, S.A. van der; Leslie, S.K. (0000-0002-4826-8642); Groves, B.; Hodge, J.A. (0000-0001-6586-8845); Popescu, C.C.; Sargent, M.T.; Schinnerer, E.; Tuffs, R.J.
Published
2022
Publication type
Article / Letter to editor
GalaxiesStar formationUltravioletGalaxies - evolutionGalaxies - ISMDustExtinctionAstrophysics - astrophysics of galaxies
Date issued
2022
Language
English
Is part of
Astronomy & Astrophysics (2022), A26
hdl
1887/3562530
doi
10.1051/0004-6361/202142452
URL
https://ui.adsabs.harvard.edu/abs/2022A&A...662A..26V