The protoplanetary system HD 100546 in Hαpolarized light from SPHERE/ZIMPOL

2017/10/31 by I. Mendigutía, R. D. Oudmaijer, A. Garufi +10
Physics and Astronomy · #Astro and Planetary Science #Astrobiology #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Biology #Context (archaeology) #Exoplanet #Physics #Planet #Planetary system #Protoplanet #Protoplanetary disk #Solar System #Stars #Stellar, planetary, and galactic studies #astro-ph.EP #astro-ph.IM #astro-ph.SR

paper · pdf · doi:10.1051/0004-6361/201731131

published as A&A 608, A104 (2017) · 8 pages, 7 figures. Accepted in A&A

arxiv created 2017/10/31 · openalex created_date 2017/11/10 · openalex publication_date 2017/12/01 · arxiv updated 2017/12/13 · openalex updated_date 2026/08/05

Abstract

Context. HD 100546 is one of the few known pre-main-sequence stars that may host a planetary system in its disk.

Citations

• High-resolution Br γ spectro-interferometry of the transitional Herbig Ae/Be star HD 100546: a Keplerian gaseous disc inside the inner rim
• Evolutionary models for cool brown dwarfs and extrasolar giant planets. The case of HD 209458
• Direct Imaging of Bridged Twin Protoplanetary Disks in a Young Multiple Star
• Flows of gas through a protoplanetary gap
• Disk Frequencies and Lifetimes in Young Clusters
• VERY LARGE TELESCOPE/NACO POLARIMETRIC DIFFERENTIAL IMAGING OF HD100546—DISK STRUCTURE AND DUST GRAIN PROPERTIES BETWEEN 10 AND 140 AU
• Resolved Observations of Transition Disks
• CO emission tracing a warp or radial flow within ≲100 au in the HD 100546 protoplanetary disk