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Adaptable Radiative Transfer Innovations for Submillimeter Telescopes (ARTIST)

Published online by Cambridge University Press:  27 April 2011

Marco Padovani ,
Jes K. Jørgensen ,
Frank Bertoldi ,
Christian Brinch ,
Pau Frau ,
Josep Miquel Girart ,
Michiel Hogerheijde ,
Attila Juhasz ,
Rolf Kuiper  and
Reinhold Schaaf
...Show all authors
Marco Padovani
Affiliation:
Institut de Ciències de l'Espai (CSIC-IEEC), Universitat Autònoma de Barcelona, Spain email: padovani@ice.cat, girart@ice.cat, frau@ice.cat
Jes K. Jørgensen
Affiliation:
Centre for Star and Planet Formation, University of Copenhagen, Denmark email: jes@snm.ku.dk
Frank Bertoldi
Affiliation:
Argelander Insitute for Astronomy, University of Bonn, Germany email: wouter@astro.uni-bonn.de, bertoldi@astro.uni-bonn.de, rschaaf@astro.uni-bonn.de, kuiper@astro.uni-bonn.de
Christian Brinch
Affiliation:
Leiden Observatory, University of Leiden, the Netherlands email: michiel@strw.leidenuniv.nl, brinch@strw.leidenuniv.nl, juhasz@strw.leidenuniv.nl
Pau Frau
Affiliation:
Institut de Ciències de l'Espai (CSIC-IEEC), Universitat Autònoma de Barcelona, Spain email: padovani@ice.cat, girart@ice.cat, frau@ice.cat
Josep Miquel Girart
Affiliation:
Institut de Ciències de l'Espai (CSIC-IEEC), Universitat Autònoma de Barcelona, Spain email: padovani@ice.cat, girart@ice.cat, frau@ice.cat
Michiel Hogerheijde
Affiliation:
Leiden Observatory, University of Leiden, the Netherlands email: michiel@strw.leidenuniv.nl, brinch@strw.leidenuniv.nl, juhasz@strw.leidenuniv.nl
Attila Juhasz
Affiliation:
Leiden Observatory, University of Leiden, the Netherlands email: michiel@strw.leidenuniv.nl, brinch@strw.leidenuniv.nl, juhasz@strw.leidenuniv.nl
Rolf Kuiper
Affiliation:
Argelander Insitute for Astronomy, University of Bonn, Germany email: wouter@astro.uni-bonn.de, bertoldi@astro.uni-bonn.de, rschaaf@astro.uni-bonn.de, kuiper@astro.uni-bonn.de
Reinhold Schaaf
Affiliation:
Argelander Insitute for Astronomy, University of Bonn, Germany email: wouter@astro.uni-bonn.de, bertoldi@astro.uni-bonn.de, rschaaf@astro.uni-bonn.de, kuiper@astro.uni-bonn.de
Wouter H. T. Vlemmings
Affiliation:
Argelander Insitute for Astronomy, University of Bonn, Germany email: wouter@astro.uni-bonn.de, bertoldi@astro.uni-bonn.de, rschaaf@astro.uni-bonn.de, kuiper@astro.uni-bonn.de
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Abstract

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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 transfermethods: numericalstars: formationsubmillimeterpolarization
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S270: Computational Star Formation , May 2010 , pp. 451 - 454
Copyright
Copyright © International Astronomical Union 2011

References

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