Determining dispersal mechanisms of protoplanetary disks using accretion and wind mass loss rates

Abstract

Understanding the origin of accretion and dispersal of protoplanetary disks is fundamental for investigating planet formation. Recent numerical simulations show that launching winds are unavoidable when disks undergo magnetically driven accretion and/or are exposed to external UV radiation. Observations also hint that disk winds are common. We explore how the resulting wind mass loss rate can be used as a probe of both disk accretion and dispersal. As a proof-of-concept study, we focus on magnetocentrifugal winds, MRI (magnetorotational instability) turbulence, and external photoevapotaion. By developing a simple, yet physically motivated disk model and coupling it with simulation results available in the literature, we compute the mass loss rate as a function of external UV flux for each mechanism. We find that different mechanisms lead to different levels of mass loss rate, indicating that the origin of disk accretion and dispersal can be determined, by observing the wind mass loss rate resulting from each mechanism. This determination provides important implications for planet formation. This work thus shows that the ongoing and future observations of the wind mass loss rate for protoplanetary disks are paramount to reliably constrain how protoplanetary disks evolve with time and how planet formation takes place in the disks.

16 pages; 7 figures, 5 tables, accepted for publication in ApJL; no change in the conclusions; the additional Monte-Carlo based, parameter study was conducted, following the referee's comment

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Cited by in corpus (8)

• The growth and migration of massive planets under the influence of external photoevaporation
• Testing external photoevaporation in the $\sigma$-Orionis cluster with spectroscopy and disk mass measurements
• ALMA Band 6 high-resolution observations of the transitional disk around SY Cha
• Photoionized Herbig-Haro objects in the Orion Nebula through deep high-spectral resolution spectroscopy III: HH514
• [OI] 6300Å emission as a probe of external photoevaporation of protoplanetary discs
• Disk Evolution Study Through Imaging of Nearby Young Stars (DESTINYS): Scattered light detection of a possible disk wind in RY Tau
• The Longest-period Young Transiting Exoplanets. A Duo of Puffy Giants inside a Debris Disk
• Dispersal of protoplanetary discs: How stellar properties and the local environment determine the pathway of evolution