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Testing giant planet formation in the transitional disk of SAO 206462 using deep VLT/SPHERE imaging

2017/02/28 by A.-L. Maire, A. -L. Maire, T. Stolker +50 · 5 citations
Physics and Astronomy · #Astro and Planetary Science #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Context (archaeology) #Debris disk #Geology #Giant planet #Physics #Planet #Planetary system #Protoplanet #Protoplanetary disk #Spiral galaxy #Stars #Stellar, planetary, and galactic studies #astro-ph.EP

paper · pdf · doi:10.1051/0004-6361/201629896

published as A&A 601, A134 (2017) · A&A, in press. 16 pages, 17 figures. Updated to match proofs

openalex publication_date 2017/03/06 · arxiv created 2017/05/03 · arxiv updated 2017/05/24 · openalex created_date 2020/11/23 · openalex updated_date 2026/08/05

Abstract

Context. The SAO 206462 (HD 135344B) disk is one of the few known transitional disks showing asymmetric features in scattered light and thermal emission. Near-infrared scattered-light images revealed two bright outer spiral arms and an inner cavity depleted in dust. Giant protoplanets have been proposed to account for the disk morphology.

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