Title of article
Adaptable Radiative Transfer Innovations for Submillimeter Telescopes (ARTIST)
Author/Authors
Marco Padovani، نويسنده , , Jes K. Jorgensen on behalf of the ARTIST team: Frank Bertoldi، نويسنده , , Christian Brinch، نويسنده , , Pau Frau، نويسنده , , Josep Miquel Girart، نويسنده , , Michiel Hogerheijde، نويسنده , , Attila Juhasz، نويسنده , , Rolf Kuiper، نويسنده , , Reinhold Schaaf، نويسنده , , Wouter H. T. Vlemmings، نويسنده ,
Issue Information
روزنامه با شماره پیاپی سال 2010
Pages
4
From page
451
To page
454
Abstract
Submillimeter observations are a key for answering many of the big questions in modern-day astrophysics, such as how stars and planets form, how galaxies evolve, and how material cycles through stars and the interstellar medium. With the upcoming large submillimeter facilities ALMA and Herschel a new window will open to study these questions. ARTIST is a project funded in context of the European ASTRONET program with the aim of developing a next generation model suite for comprehensive multi-dimensional radiative transfer calculations of the dust and line emission, as well as their polarization, to help interpret observations with these groundbreaking facilities.
Keywords
radiative transfer , methods: numerical , stars: formation , polarization , Submillimeter
Journal title
Proceedings of the International Astronomical Union
Serial Year
2010
Journal title
Proceedings of the International Astronomical Union
Record number
667720
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