The Ophiuchus DIsk Survey Employing ALMA (ODISEA): Complete Size Distributions for the 100 Brightest Disks across Multiplicity and Spectral Energy Distribution Classes

The size of a protoplanetary disk is a fundamental property, yet most remain unresolved, even in nearby star-forming regions ( d ∼ 140–200 pc). We present the complete continuum size distribution for the 105 brightest protoplanetary disks ( M _dust ≳ 2 M _⊕ ) in the Ophiuchus cloud, obtained from...

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Bibliographic Details
Main Authors:	Anuroop Dasgupta, Lucas A. Cieza, Camilo González-Ruilova, Trisha Bhowmik, Prachi Chavan, Grace Batalla-Falcon, Gregory Herczeg, Dary Ruiz-Rodriguez, Jonathan P. Williams, Anibal Sierra, Simon Casassus, Octavio Guilera, Sebastian Pérez, Santiago Orcajo, P.H. Nogueira, A.S Hales, J.M. Miley, Fernando R. Rannou, Alice Zurlo
Format:	Article
Language:	English
Published:	IOP Publishing 2025-01-01
Series:	The Astrophysical Journal Letters
Subjects:	Protoplanetary disks Planetary system formation Pre-main sequence stars Submillimeter astronomy
Online Access:	https://doi.org/10.3847/2041-8213/adb03c
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The Ophiuchus DIsk Survey Employing ALMA (ODISEA): Complete Size Distributions for the 100 Brightest Disks across Multiplicity and Spectral Energy Distribution Classes

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