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arXiv · 2409.11485

Survey of Orion Disks with ALMA (SODA) III: Disks in wide binary systems in L1641 and L1647

Giulia Ricciardi·Sierk E. van Terwisga·Veronica Roccatagliata·Alvaro Hacar·Thomas Henning·Walter Del Pozzo
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Abstract

Aims. The goal of this work is to comprehensively characterize the impact of stellar multiplicity on Class II disks in the L1641 and L1647 regions of Orion A (~1-3 Myr), part of the Survey of Orion Disks with ALMA (SODA). We characterize the protostellar multiplicity using the Atacama Large Millimeter/submillimeter Array (ALMA), the ESO-VISTA, and Hubble Space telescopes. The resulting sample of 65 multiple systems represents the largest catalogue of wide binary systems to date (projected separation >1000 AU), allowing a more robust statistical characterization of the evolution and properties of protoplanetary disks. Methods. The disk population was observed in continuum with ALMA at 225 GHz, with a median rms of 1.5 Mearth. Combining these data (resolution ~1.1arcsec ) with the ESO-VISTA near-infrared survey of the Orion A cloud (resolution ~0.7arcsec ), multiple systems are assembled and selected by an iterative inside-out search in projected separation (>1000 AU). Results. We identify 61 binary systems, 3 triple systems, and one quadruple system. The separation range is between 1000 and 10^4 AU. The dust mass distributions inferred with the Kaplan-Meier estimator yield a median mass of 3.23+0.6-0.4 Mearth for primary disks and 3.88+0.3-0.3 Mearth for secondary disks.

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Giulia Ricciardi, Sierk E. van Terwisga, Veronica Roccatagliata, Alvaro Hacar, Thomas Henning, Walter Del Pozzo. 2024-09-17. Survey of Orion Disks with ALMA (SODA) III: Disks in wide binary systems in L1641 and L1647. https://doi.org/10.1051/0004-6361%2F202452287

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