RADMC-3D: A multi-purpose radiative transfer tool

By C. Dullemond, A. Juhász, A. Pohl, F. Sereshti, R. Shetty, Thomas Peters, B. Commerçon, M. Flock. 2012

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Citations in the corpus

Discovery of a planetary-mass companion within the gap of the transition disk around PDS 70 (2018, methodology): “The scattering mode in RADMC-3D was set to anisotropic scattering with full treatment A44, page 8 of 21 M. Keppler et al.: Discovery of a planetary-mass companion around PDS 70 1.0 0.5 0 -0.5 -1.0 RA [arcsec] -1.0 -0.5 0 0.5 1.0 D E C [ a rc s e c ] -100 -50 0 50 100 y [A U ] -100 -50 0 50 100 x [AU”
On planet formation in HL Tau (2015, methodology): “We perform simulated observations of our model using the RADMC-3D Monte Carlo radiative transfer code (Dullemond 2012) together with the Common Astronomy Software Application (CASA) ALMA simulator (version 4.1), focussing on ALMA band 6 (continuum emission at 233 GHz).”
The VLA/ALMA Nascent Disk and Multiplicity (VANDAM) Survey of Orion Protostars. II. A Statistical Characterization of Class 0 and Class I Protostellar Disks (2020, methodology): “We used the Monte Carlo dust radiative transfer code RADMC-3D (Dullemond et al. 2012) to compute the temperature throughout the disk embedded within an envelope. The dust opacities in our model were parameterized by the maximum grain size (see Table 11) following the method outlined by Woitke et al.”
Gaps and Rings in an ALMA Survey of Disks in the Taurus Star-forming Region (2018, unknown): “…and re-condense onto dust outside the ice line, both leading to enhanced grain growth 9 In order to derive the midplane temperature proﬁle, we use the RADMC-3D code (Dullemond et al. 2012) to run radiative transfer models with steller properties ﬁxed to the values given in Table 2 for each object.”
RINGED SUBSTRUCTURE AND A GAP AT 1 au IN THE NEAREST PROTOPLANETARY DISK (2016, background): “In principle, a single low-mass planet at ∼40 AU could potentially open a ‘double-gap’ feature if the disk is particularly inviscid (e.g., Goodman & Rafikov 2001; Dong et al. 2011; Duffell & MacFadyen 2012).”
Astrochemistry and compositions of planetary systems (2020, background): “The reader is referred to the following references: Hogerheijde and van der Tak (2000), Brinch and Hogerheijde (2010), van der Tak (2011),Dullemond et al. (2012), and Shirley (2015) 1.3.2.”