Molecules with ALMA at Planet-forming Scales (MAPS). VIII. CO Gap in AS 209-Gas Depletion or Chemical Processing? - Archive ouverte HAL Access content directly
Journal Articles The Astrophysical Journal Supplement Series Year : 2021

Molecules with ALMA at Planet-forming Scales (MAPS). VIII. CO Gap in AS 209-Gas Depletion or Chemical Processing?

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Felipe Alarcón
  • Function : Author
Arthur D. Bosman
  • Function : Author
Edwin A. Bergin
  • Function : Author
Ke Zhang
  • Function : Author
Richard Teague
Jaehan Bae
Yuri Aikawa
Sean M. Andrews
  • Function : Author
Alice S. Booth
  • Function : Author
Jenny K. Calahan
  • Function : Author
Gianni Cataldi
  • Function : Author
Ian Czekala
  • Function : Author
Jane Huang
  • Function : Author
John D. Ilee
  • Function : Author
Charles J. Law
  • Function : Author
Yao Liu
  • Function : Author
Feng Long
  • Function : Author
Ryan A. Loomis
  • Function : Author
Karin I. Öberg
  • Function : Author
Kamber R. Schwarz
  • Function : Author
Merel L. R. Van'T Hoff
  • Function : Author
Catherine Walsh
  • Function : Author
David J. Wilner
  • Function : Author

Abstract

Emission substructures in gas and dust are common in protoplanetary disks. Such substructures can be linked to planet formation or planets themselves. We explore the observed gas substructures in AS 209 using thermochemical modeling with RAC2D and high-spatial-resolution data from the Molecules with ALMA at Planet-forming Scales (MAPS) program. The observations of C18O J = 2-1 emission exhibit a strong depression at 88 au overlapping with the positions of multiple gaps in millimeter dust continuum emission. We find that the observed CO column density is consistent with either gas surface-density perturbations or chemical processing, while C2H column density traces changes in the C/O ratio rather than the H2 gas surface density. However, the presence of a massive planet (>0.2 MJup) would be required to account for this level of gas depression, which conflicts with constraints set by the dust emission and the pressure profile measured by gas kinematics. Based on our models, we infer that a local decrease of CO abundance is required to explain the observed structure in CO, dominating over a possible gap-carving planet present and its effect on the H2 surface density. This paper is part of the MAPS special issue of the Astrophysical Journal Supplement.

Dates and versions

insu-03672373 , version 1 (19-05-2022)

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Felipe Alarcón, Arthur D. Bosman, Edwin A. Bergin, Ke Zhang, Richard Teague, et al.. Molecules with ALMA at Planet-forming Scales (MAPS). VIII. CO Gap in AS 209-Gas Depletion or Chemical Processing?. The Astrophysical Journal Supplement Series, 2021, 257, ⟨10.3847/1538-4365/ac22ae⟩. ⟨insu-03672373⟩
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