Organic molecules in the protoplanetary disk of DG Tauri revealed by ALMA

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Title: Organic molecules in the protoplanetary disk of DG Tauri revealed by ALMA
Authors: Podio, LindaBacciotti, FrancescaFedele, D.Coffey, Deirdre
Permanent link: http://hdl.handle.net/10197/11141
Date: 8-Mar-2019
Online since: 2019-10-11T14:42:00Z
Abstract: Context. Planets form in protoplanetary disks and inherit their chemical compositions. Aims. It is thus crucial to map the distribution and investigate the formation of simple organics, such as formaldehyde and methanol, in protoplanetary disks. Methods. We analyze ALMA observations of the nearby disk-jet system around the T Tauri star DG Tau in the o-H2CO 31, 2-21, 1 and CH3OH 3-2, 2-4-1, 4 E, 50, 5-40, 4 A transitions at an unprecedented resolution of $ ∼0.15 $, i.e., ∼18 au at a distance of 121 pc. Results. The H2CO emission originates from a rotating ring extending from ∼40 au with a peak at ∼62 au, i.e., at the edge of the 1.3 mm dust continuum. CH3OH emission is not detected down to an rms of 3 mJy beam-1 in the 0.162 km s-1 channel. Assuming an ortho-to-para ratio of 1.8-2.8 the ring-and disk-height-averaged H2CO column density is ∼0.3-4 × 1014 cm-2, while that of CH3OH is < 0.04-0.7 × 1014 cm-2. In the inner 40 au no o-H2CO emission is detected with an upper limit on its beam-averaged column density of ∼0.5-6 × 1013 cm-2. Conclusions. The H2CO ring in the disk of DG Tau is located beyond the CO iceline (RCO ∼ 30 au). This suggests that the H2CO abundance is enhanced in the outer disk due to formation on grain surfaces by the hydrogenation of CO ice. The emission peak at the edge of the mm dust continuum may be due to enhanced desorption of H2CO in the gas phase caused by increased UV penetration and/or temperature inversion. The CH3OH/H2CO abundance ratio is < 1, in agreement with disk chemistry models. The inner edge of the H2CO ring coincides with the radius where the polarization of the dust continuum changes orientation, hinting at a tight link between the H2CO chemistry and the dust properties in the outer disk and at the possible presence of substructures in the dust distribution.
metadata.dc.description.othersponsorship: PRIN-INAF/2016 GENISIS-SKA
Italian Ministero dell-Istruzione
Università e Ricera
Swiss National Science Foundation
Type of material: Journal Article
Publisher: EDP Sciences
Journal: Astronomy and Astrophysics
Volume: 623
Copyright (published version): 2019 ESO
Keywords: Protoplanetary disksAstrochemistryDG Tau
DOI: 10.1051/0004-6361/201834475
Language: en
Status of Item: Peer reviewed
Appears in Collections:Physics Research Collection

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