Standard
Adaptable radiative transfer innovations for submillimeter telescopes (ARTIST). / Padovani, Marco; Jørgensen, Jes Kristian; Bertoldi, Frank; Brinch, Christian; Frau, Pau; Girart, Josep Miquel; Hogerheijde, Michiel; Juhasz, Attila; Kuiper, Rolf; Schaaf, Reinhold; Vlemmings, Wouter H. T.
Computational Star Formation: proceedings of the Twenty Seventh General Assembly Rio de Janeiro 2009. ed. / João Alves; Bruce G. Elmegreen; Josep M. Girart; Virginia Trimble. Cambridge University Press, 2011. p. 451-454 (Proceedings of the International Astronomical Union; No. S270, Vol. 6).
Research output: Chapter in Book/Report/Conference proceeding › Article in proceedings › Research › peer-review
Harvard
Padovani, M
, Jørgensen, JK, Bertoldi, F, Brinch, C, Frau, P, Girart, JM, Hogerheijde, M, Juhasz, A, Kuiper, R, Schaaf, R & Vlemmings, WHT 2011,
Adaptable radiative transfer innovations for submillimeter telescopes (ARTIST). in J Alves, BG Elmegreen, JM Girart & V Trimble (eds),
Computational Star Formation: proceedings of the Twenty Seventh General Assembly Rio de Janeiro 2009. Cambridge University Press, Proceedings of the International Astronomical Union, no. S270, vol. 6, pp. 451-454, 27th General Assembly of the International Astronomical Union, Rio de Janeiro, Brazil,
03/08/2009.
https://doi.org/10.1017/S1743921311000792APA
Padovani, M.
, Jørgensen, J. K., Bertoldi, F., Brinch, C., Frau, P., Girart, J. M., Hogerheijde, M., Juhasz, A., Kuiper, R., Schaaf, R., & Vlemmings, W. H. T. (2011).
Adaptable radiative transfer innovations for submillimeter telescopes (ARTIST). In J. Alves, B. G. Elmegreen, J. M. Girart, & V. Trimble (Eds.),
Computational Star Formation: proceedings of the Twenty Seventh General Assembly Rio de Janeiro 2009 (pp. 451-454). Cambridge University Press. Proceedings of the International Astronomical Union Vol. 6 No. S270
https://doi.org/10.1017/S1743921311000792Vancouver
Padovani M
, Jørgensen JK, Bertoldi F, Brinch C, Frau P, Girart JM et al.
Adaptable radiative transfer innovations for submillimeter telescopes (ARTIST). In Alves J, Elmegreen BG, Girart JM, Trimble V, editors, Computational Star Formation: proceedings of the Twenty Seventh General Assembly Rio de Janeiro 2009. Cambridge University Press. 2011. p. 451-454. (Proceedings of the International Astronomical Union; No. S270, Vol. 6).
https://doi.org/10.1017/S1743921311000792Author
Padovani, Marco ; Jørgensen, Jes Kristian ; Bertoldi, Frank ; Brinch, Christian ; Frau, Pau ; Girart, Josep Miquel ; Hogerheijde, Michiel ; Juhasz, Attila ; Kuiper, Rolf ; Schaaf, Reinhold ; Vlemmings, Wouter H. T. / Adaptable radiative transfer innovations for submillimeter telescopes (ARTIST). Computational Star Formation: proceedings of the Twenty Seventh General Assembly Rio de Janeiro 2009. editor / João Alves ; Bruce G. Elmegreen ; Josep M. Girart ; Virginia Trimble. Cambridge University Press, 2011. pp. 451-454 (Proceedings of the International Astronomical Union; No. S270, Vol. 6).
Bibtex
@inproceedings{2005799e818843c78e29f49410ae6f29,
title = "Adaptable radiative transfer innovations for submillimeter telescopes (ARTIST)",
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 = "methods: numerical, polarization, radiative transfer, stars: formation, submillimeter",
author = "Marco Padovani and J{\o}rgensen, {Jes Kristian} and Frank Bertoldi and Christian Brinch and Pau Frau and Girart, {Josep Miquel} and Michiel Hogerheijde and Attila Juhasz and Rolf Kuiper and Reinhold Schaaf and Vlemmings, {Wouter H. T.}",
year = "2011",
month = apr,
doi = "10.1017/S1743921311000792",
language = "English",
isbn = "9780521766432",
series = "Proceedings of the International Astronomical Union",
publisher = "Cambridge University Press",
number = "S270",
pages = "451--454",
editor = "Jo{\~a}o Alves and Elmegreen, {Bruce G.} and Girart, {Josep M.} and Virginia Trimble",
booktitle = "Computational Star Formation",
address = "United Kingdom",
note = "27th General Assembly of the International Astronomical Union ; Conference date: 03-08-2009 Through 14-08-2009",
}
RIS
TY - GEN
T1 - Adaptable radiative transfer innovations for submillimeter telescopes (ARTIST)
AU - Padovani, Marco
AU - Jørgensen, Jes Kristian
AU - Bertoldi, Frank
AU - Brinch, Christian
AU - Frau, Pau
AU - Girart, Josep Miquel
AU - Hogerheijde, Michiel
AU - Juhasz, Attila
AU - Kuiper, Rolf
AU - Schaaf, Reinhold
AU - Vlemmings, Wouter H. T.
N1 - Conference code: 27
PY - 2011/4
Y1 - 2011/4
N2 - 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.
AB - 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.
KW - methods: numerical
KW - polarization
KW - radiative transfer
KW - stars: formation
KW - submillimeter
UR - http://www.scopus.com/inward/record.url?scp=79956225943&partnerID=8YFLogxK
U2 - 10.1017/S1743921311000792
DO - 10.1017/S1743921311000792
M3 - Article in proceedings
AN - SCOPUS:79956225943
SN - 9780521766432
T3 - Proceedings of the International Astronomical Union
SP - 451
EP - 454
BT - Computational Star Formation
A2 - Alves, João
A2 - Elmegreen, Bruce G.
A2 - Girart, Josep M.
A2 - Trimble, Virginia
PB - Cambridge University Press
T2 - 27th General Assembly of the International Astronomical Union
Y2 - 3 August 2009 through 14 August 2009
ER -
