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A New Raytracer for Modeling AU-Scale Imaging of Lines from Protoplanetary Disks

Pontoppidan, Klaus M. and Meijerink, Rowin and Dullemond, Cornelis P. and Blake, Geoffrey A. (2009) A New Raytracer for Modeling AU-Scale Imaging of Lines from Protoplanetary Disks. Astrophysical Journal, 704 (2). pp. 1482-1494. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:20091023-113327332

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Abstract

The material that formed the present-day solar system originated in feeding zones in the inner solar nebula located at distances within ~20 AU from the Sun, known as the planet-forming zone. Meteoritic and cometary material contain abundant evidence for the presence of a rich and active chemistry in the planet-forming zone during the gas-rich phase of solar system formation. It is a natural conjecture that analogs can be found among the zoo of protoplanetary disks around nearby young stars. The study of the chemistry and dynamics of planet formation requires: (1) tracers of dense gas at 100-1000 K and (2) imaging capabilities of such tracers with 5-100 mas (0.5-20 AU) resolution, corresponding to the planet-forming zone at the distance of the closest star-forming regions. Recognizing that the rich infrared (2-200 μm) molecular spectrum recently discovered to be common in protoplanetary disks represents such a tracer, we present a new general ray-tracing code, RADLite, that is optimized for producing infrared line spectra and images from axisymmetric structures. RADLite can consistently deal with a wide range of velocity gradients, such as those typical for the inner regions of protoplanetary disks. The code is intended as a back-end for chemical and excitation codes, and can rapidly produce spectra of thousands of lines for grids of models for comparison with observations. Such radiative transfer tools will be crucial for constraining both the structure and chemistry of planet-forming regions, including data from current infrared imaging spectrometers and extending to the Atacama Large Millimeter Array and the next generation of Extremely Large Telescopes, the James Webb Space Telescope and beyond.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1088/0004-637X/704/2/1482DOIArticle
http://www.iop.org/EJ/abstract/0004-637X/704/2/1482/PublisherArticle
ORCID:
AuthorORCID
Pontoppidan, Klaus M.0000-0001-7552-1562
Blake, Geoffrey A.0000-0003-0787-1610
Additional Information:© 2009 American Astronomical Society. Received 2009 July 2; accepted 2009 September 8; published 2009 October 2. An anonymous referee provided a thorough and constructive report that improved the manuscript considerably. The authors are grateful to Sarah Kendrew, Leiden Observatory, for providing a high-resolution infrared transmission spectrum model. Discussions with Joan Najita, Colette Salyk, and Marco Spaans have been valuable during the preparation of the manuscript. Support for K.M.P. was provided by NASA through Hubble Fellowship grant #01201.01 awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract NAS 5-26555. R.M. has been supported by NSF grant AST-0708922.
Funders:
Funding AgencyGrant Number
NASA Hubble Fellowship01201.01
NSFAST-0708922
Subject Keywords:astrochemistry; planetary systems: protoplanetary disks; radiative transfer; techniques: high angular resolution
Issue or Number:2
Record Number:CaltechAUTHORS:20091023-113327332
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20091023-113327332
Official Citation:A New Raytracer for Modeling AU-Scale Imaging of Lines from Protoplanetary Disks Klaus M. Pontoppidan, Rowin Meijerink, Cornelis P. Dullemond, and Geoffrey A. Blake 2009 ApJ 704 1482-1494 doi: 10.1088/0004-637X/704/2/1482
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:16470
Collection:CaltechAUTHORS
Deposited By: Jason Perez
Deposited On:23 Oct 2009 20:34
Last Modified:03 Oct 2019 01:12

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