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Dust production scenarios in galaxies at z ~ 6-8.3
Astronomy and Astrophysics
The mechanism of dust formation in galaxies at high redshift is still unknown. Asymptotic giant branch (AGB) stars and explosions of supernovae (SNe) are possible dust producers, and non-stellar processes may substantially contribute to dust production, for example grain growth in the interstellar medium (ISM). Our aim is to determine the contribution to dust production of AGB stars and SNe in nine galaxies at z ~ 6-8.3, for which observations of dust have been recently attempted. In order todoi:10.1051/0004-6361/201935149 fatcat:gibyjy4pubblvdom4btnvc7i5m