Multiwavelength analysis for interferometric (sub-)mm observations of protoplanetary disks

2015/12/17 by Marco Tazzari, M. Tazzari, L. Testi +38 · 13 citations
Chemistry · Physics and Astronomy · #Astrophysics #Astrophysics and Star Formation Studies #Galaxy #Grain size #Interferometry #Materials science #Molecular Spectroscopy and Structure #Opacity #Optics #Physics #Planet #Plateau de Bure Interferometer #Protoplanetary disk #RADIUS #Star formation #Stellar, planetary, and galactic studies #Wavelength #astro-ph.EP #astro-ph.GA #astro-ph.SR

paper · pdf · doi:10.1051/0004-6361/201527423

published as A&A 588, A53 (2016) · 19 pages, 15 figures, accepted for publication in A&A

arxiv created 2015/12/17 · openalex publication_date 2016/02/04 · arxiv updated 2016/03/23 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Context. The growth of dust grains from sub-μm to mm and cm sizes is the first step towards the formation of planetesimals. Theoretical models of grain growth predict that dust properties change as a function of disk radius, mass, age, and other physical conditions. High angular resolution observations at several (sub-)mm wavelengths constitute the ideal tool with which to directly probe the bulk of dust grains and to investigate the radial distribution of their properties.

Citations

• The size distribution of interstellar grains
• Berechnung verschiedener physikalischer Konstanten von heterogenen Substanzen. I. Dielektrizitätskonstanten und Leitfähigkeiten der Mischkörper aus isotropen Substanzen
• Passive Irradiated Circumstellar Disks with an Inner Hole
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• Constraints on Properties of the Protoplanetary Disks around UX Orionis and CQ Tauri
• emcee: The MCMC Hammer
• Formation of the Terrestrial Planets
• GRAIN GROWTH IN THE CIRCUMSTELLAR DISKS OF THE YOUNG STARS CY Tau AND DoAr 25

Cited by

• Dust masses of young disks: constraining the initial solid reservoir for planet formation
• Observing protoplanetary discs with the Square Kilometre Array – I. Characterizing pebble substructure caused by forming planets
• Asymmetric mid-plane gas in ALMA images of HD 100546
• Measurement of Circumstellar Disk Sizes in the Upper Scorpius OB Association with ALMA
• New Insights into the Nature of Transition Disks from a Complete Disk Survey of the Lupus Star-forming Region
• THE VLA VIEW OF THE HL TAU DISK: DISK MASS, GRAIN EVOLUTION, AND EARLY PLANET FORMATION
• Emission from Magnetized Accretion Disks around Young Stars
• Stellar multiplicity affects the correlation between proto-planetary disc masses and accretion rates: binaries explain high-accretors in Upper Sco
• How do T Tauri stars accrete?
• GALARIO: a GPU accelerated library for analysing radio interferometer observations
• Demographics of disks around young very low-mass stars and brown dwarfs in Lupus
• A balanced budget view on forming giant planets by pebble accretion
• A Brief Overview of Planet Formation