High-redshift objects in dust environments

Details High-redshift objects in dust environments High-redshift objects in dust environments

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011rmxac..40...70m&link_type=abstract

XIII Latin American Regional IAU Meeting (Eds. W. J. Henney & S. Torres-Peimbert) Revista Mexicana de Astronomía y Astrofísica (

Astronomy and Astrophysics

Astronomy

Cosmology: Observations, Dust, Extinction, Early Universe, Galaxies: Evolution

Scientific paper

We give an introduction for a project related to the study of high-redshift objects (mainly star forming galaxies) which may harbor large amounts of dust within them. The incoming of better and powerful telescopes in the infrared and submillimeter wavelengths (e.g., ALMA, JWST), together with stellar population synthesis models, radiative transfer models, and dust evolution models will help to unmask the cosmic evolution of dust content in galaxies.

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