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Journal Articles The Astronomical Journal Year : 2021

Characterizing the Protolunar Disk of the Accreting Companion GQ Lupi B

Tomas Stolker
  • Function : Author
Sebastiaan Y. Haffert
  • Function : Author
Aurora Y. Kesseli
  • Function : Author
Rob G. van Holstein
  • Function : Author
Yuhiko Aoyama
  • Function : Author
Jarle Brinchmann
  • Function : Author
Gabriele Cugno
  • Function : Author
Julien H. Girard
  • Function : Author
Gabriel-Dominique Marleau
  • Function : Author
Michael R. Meyer
  • Function : Author
Sascha P. Quanz
  • Function : Author
Ignas A. G. Snellen
  • Function : Author
Kamen O. Todorov
  • Function : Author

Abstract

GQ Lup B is a young and accreting, substellar companion that appears to drive a spiral arm in the circumstellar disk of its host star. We report high-contrast imaging observations of GQ Lup B with VLT/NACO at 4-5 μm and medium-resolution integral field spectroscopy with VLT/MUSE. The optical spectrum is consistent with an M9 spectral type, shows characteristics of a low-gravity atmosphere, and exhibits strong Hα emission. The H - M' color is ≳1 mag redder than field dwarfs with similar spectral types, and a detailed analysis of the spectral energy distribution (SED) from optical to mid-infrared wavelengths reveals excess emission in the L', NB4.05, and M' bands. The excess flux is well described by a blackbody component with T disk ≍ 460 K and R disk ≍ 65 R J and is expected to trace continuum emission from small grains in a protolunar disk. We derive an extinction of A V ≍ 2.3 mag from the broadband SED with a suspected origin in the vicinity of the companion. We also combine 15 yr of astrometric measurements and constrain the mutual inclination with the circumstellar disk to 84 ± 9 deg, indicating a tumultuous dynamical evolution or a stellar-like formation pathway. From the measured Hα flux and the estimated companion mass, M p ≍ 30 M J, we derive an accretion rate of $\dot{M}\approx {10}^{-6.5}\,{M}_{{\rm{J}}}\,{\mathrm{yr}}^{-1}$ . We speculate that the disk is in a transitional stage in which the assembly of satellites from a pebble reservoir has opened a central cavity while GQ Lup B is in the final stages of its formation. ∗Based on observations collected under ESO programmes 0101.C-0502(B), 0102.C-0649(A), and 0103.C-0524(A).

Dates and versions

insu-03705258 , version 1 (27-06-2022)

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Cite

Tomas Stolker, Sebastiaan Y. Haffert, Aurora Y. Kesseli, Rob G. van Holstein, Yuhiko Aoyama, et al.. Characterizing the Protolunar Disk of the Accreting Companion GQ Lupi B. The Astronomical Journal, 2021, 162, ⟨10.3847/1538-3881/ac2c7f⟩. ⟨insu-03705258⟩
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