Shadows and spirals in the protoplanetary disk HD 100453

By M. Benisty, T. Stolker, A. Pohl, J. D. Boer, G. Lesur, C. Dominik, C. Dullemond, Maud Langlois, M. Min, K. Wagner and 39 more. 2016

139 citations recorded by the source corpus.

ESO; CNRS (France); MPIA (Germany); INAF (Italy); FINES (Switzerland); NOVA (Netherlands); European Commission, Optical Infrared Coordination Network for Astronomy (OPTICON) [RII3-Ct-2004-001566, 226604, 312430]; Programme National de Planetologie (PNP); Programme National de Physique Stellaire (PNPS) of CNRS-INSU; French Labex OSUG@2020 (Investissements d'avenir) [ANR10 LABX56]; NASA's Science Mission Directorate; DISCSIM project - European Research Council [341137]; Italian Ministry of Education, University, and Research

Subfields: Astronomy and Astrophysics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/b38f78b73a87f2b8135f51ebdfd683084c02a852

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. T. Birnstiel
2. D. Wilner
3. S. Andrews
4. Matthew R. Bate
5. Xue-Ning Bai
6. C. Dullemond
7. Zhaohuan Zhu
8. L. Ricci

In Instrumentation

1. S. Andrews
2. T. Birnstiel
3. D. Wilner
4. Xue-Ning Bai
5. Zhaohuan Zhu
6. Matthew R. Bate
7. L. P'erez
8. J. Carpenter

Citations in the corpus

• SPHERE: the exoplanet imager for the Very Large Telescope (2019, background): “…of circumstellar scattered light, mainly dust scattering from circumstellar disks around young stars (e.g., Garufi et al. 2016; Stolker et al. 2016; Benisty et al. 2017; van Boekel et al. 2017), but also dust scattering in the wind of mass loosing red giants and supergiants (Khouri et al. 2016;…”
• The Disk Substructures at High Angular Resolution Project (DSHARP). VI. Dust Trapping in Thin-ringed Protoplanetary Disks (2018, background): “But these transitional disks seem to be rather violent environments, possibly with strong warps (Marino et al. 2015; Benisty et al. 2017) and companion-induced spirals (Dong et al. 2016).”
• On the diversity and statistical properties of protostellar discs (2018, background): “In the absence of more information it is difficult to know whether observed spiral structure is generated by a companion (as in the case of HD 100453; Wagner et al. 2015; Dong et al. 2016; Benisty et al. 2017) or disc self gravity.”