An updated dust-to-star geometry: dust attenuation does not depend on inclination in 1.3 ≤ z ≤ 2.6 star-forming galaxies from MOSDEF

Author(s):
Lorenz, B.; Kriek, M.T.; Shapley, A.E.; Reddy, N.A.; Sanders, R.L.; Barro, G.; Coil, A.L.; Mobasher, B.; Price, S.H.; Runco, J.N.; Shivaei, I.; Siana, B.; Weisz, D.R.
Published
2023
Publication type
Article / Letter to editor
Galaxy propertiesGalaxy evolutionHigh-redshift galaxiesStar formation6155947341569Astrophysics - Astrophysics of Galaxies
Date issued
2023
Language
English
Is part of
The Astrophysical Journal (2023), No. 1, 29
hdl
1887/3715301
doi
10.3847/1538-4357/accdd1
URL
https://ui.adsabs.harvard.edu/abs/2023ApJ...951...29L