The Origin and Fate of Dust in Our Universe

Forskningsprojekt, 2020 – 2026

Beskrivning saknas.

Deltagare

Samarbetspartners

Finansiering

Publikationer

A dusty protocluster surrounding the binary galaxy HerBS-70 at z = 2.3

An empirical view of the extended atmosphere and inner envelope of the asymptotic giant branch star R Doradus I. Physical model based on CO lines

Modeling Dust Production, Growth, and Destruction in Reionization-era Galaxies with the CROC Simulations. II. Predicting the Dust Content of High-redshift Galaxies

Mer information

Projektet på Chalmers webb

https://www.chalmers.se/en/departments/see...

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