%0 Generic %1 Padovani2011 %A Padovani, Marco %A Jørgensen, Jes %A for the ARTIST Collaboration, %D 2011 %K RadTran code dust molecules %T Adaptable Radiative Transfer Innovations for Submillimeter Telescopes (ARTIST) %U http://arxiv.org/abs/1102.4815 %X 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.

@misc{Padovani2011, 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. }, added-at = {2011-02-24T19:46:37.000+0100}, author = {Padovani, Marco and Jørgensen, Jes and for the ARTIST Collaboration}, biburl = {https://www.bibsonomy.org/bibtex/24978d08bd9fb68d837cc19e1973d7d77/miki}, description = {[1102.4815] Adaptable Radiative Transfer Innovations for Submillimeter Telescopes (ARTIST)}, interhash = {7f02860ec96aaf2082795bc9815f6e04}, intrahash = {4978d08bd9fb68d837cc19e1973d7d77}, keywords = {RadTran code dust molecules}, note = {cite arxiv:1102.4815 Comment: 4 pages, 1 figure; to appear in "IAU Symposium 270: Computational Star formation", Eds. J. Alves, B. Elmegreen, J. Girart, V. Trimble}, timestamp = {2011-02-24T19:46:37.000+0100}, title = {Adaptable Radiative Transfer Innovations for Submillimeter Telescopes (ARTIST)}, url = {http://arxiv.org/abs/1102.4815}, year = 2011 }