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Cited article:
R. Siebenmorgen, F. Heymann
A&A, 539 (2012) A20
Published online: 2012-02-20
This article has been cited by the following article(s):
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GPU-BASED MONTE CARLO DUST RADIATIVE TRANSFER SCHEME APPLIED TO ACTIVE GALACTIC NUCLEI
Frank Heymann and Ralf Siebenmorgen
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Extinction and dust properties in a clumpy medium
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Polycyclic aromatic hydrocarbons in protoplanetary disks: emission and X-ray destruction
R. Siebenmorgen and F. Heymann
Astronomy & Astrophysics 543 A25 (2012)
DOI: 10.1051/0004-6361/201219039
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DUST EVOLUTION CAN PRODUCE SCATTERED LIGHT GAPS IN PROTOPLANETARY DISKS
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The Astrophysical Journal 813 (1) L14 (2015)
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Turbulent thermal diffusion: a way to concentrate dust in protoplanetary discs
Alexander Hubbard
Monthly Notices of the Royal Astronomical Society 456 (3) 3079 (2016)
DOI: 10.1093/mnras/stv2895
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THE EFFECTS OF SELF-SHADOWING BY A PUFFED-UP INNER RIM IN SCATTERED LIGHT IMAGES OF PROTOPLANETARY DISKS
Ruobing Dong (董若冰)
The Astrophysical Journal 810 (1) 6 (2015)
DOI: 10.1088/0004-637X/810/1/6
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Effect of dust grain porosity on the appearance of protoplanetary disks
F. Kirchschlager and S. Wolf
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TIME EVOLUTION OF A VISCOUS PROTOPLANETARY DISK WITH A FREE GEOMETRY: TOWARD A MORE SELF-CONSISTENT PICTURE
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The Astrophysical Journal 786 (1) 35 (2014)
DOI: 10.1088/0004-637X/786/1/35
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Self-consistent two-phase AGN torus models
Ralf Siebenmorgen, Frank Heymann and Andreas Efstathiou
Astronomy & Astrophysics 583 A120 (2015)
DOI: 10.1051/0004-6361/201526034
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Surface waves in protoplanetary disks induced by outbursts: Concentric rings in scattered light
A. D. Schneider, C. P. Dullemond and B. Bitsch
Astronomy & Astrophysics 617 L7 (2018)
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