Adaptable radiative transfer innovations for submillimeter telescopes (ARTIST)

Marco Padovani*, Jes Kristian Jørgensen, Frank Bertoldi, Christian Brinch, Pau Frau, Josep Miquel Girart, Michiel Hogerheijde, Attila Juhasz, Rolf Kuiper, Reinhold Schaaf, Wouter H. T. Vlemmings

*Corresponding author af dette arbejde
1 Citationer (Scopus)

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.

OriginalsprogEngelsk
TitelComputational Star Formation : proceedings of the Twenty Seventh General Assembly Rio de Janeiro 2009
RedaktørerJoão Alves, Bruce G. Elmegreen, Josep M. Girart, Virginia Trimble
Antal sider4
ForlagCambridge University Press
Publikationsdatoapr. 2011
Sider451-454
ISBN (Trykt)9780521766432
DOI
StatusUdgivet - apr. 2011
Begivenhed27th General Assembly of the International Astronomical Union - Rio de Janeiro, Brasilien
Varighed: 3 aug. 200914 aug. 2009
Konferencens nummer: 27

Konference

Konference27th General Assembly of the International Astronomical Union
Nummer27
Land/OmrådeBrasilien
ByRio de Janeiro
Periode03/08/200914/08/2009
NavnProceedings of the International Astronomical Union
NummerS270
Vol/bind6
ISSN1743-9213

Emneord

  • methods: numerical
  • polarization
  • radiative transfer
  • stars: formation
  • submillimeter

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