Authors

William O. Balmer, Johns Hopkins University
Laurent Pueyo, Space Telescope Science Institute
Tomas Stolker, Sterrewacht Leiden
Henrique Reggiani, Carnegie Observatories
A. L. Maire, Université de Liège
S. Lacour, LESIA - Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique
P. Mollière, Max Planck Institute for Astronomy
M. Nowak, Institute of Astronomy
D. Sing, Johns Hopkins University
N. Pourré, Institut de Planétologie et d’Astrophysique de Grenoble (IPAG)
S. Blunt, California Institute of Technology
J. J. Wang, Northwestern University
E. Rickman, European Space Agency - ESA
J. Kammerer, Space Telescope Science Institute
Th Henning, Max Planck Institute for Astronomy
K. Ward-Duong, Smith CollegeFollow
R. Abuter, European Southern Observatory
A. Amorim, Faculdade de Ciências da Universidade de Lisboa
R. Asensio-Torres, Max Planck Institute for Astronomy
M. Benisty, Institut de Planétologie et d’Astrophysique de Grenoble (IPAG)
J. P. Berger, Institut de Planétologie et d’Astrophysique de Grenoble (IPAG)
H. Beust, Institut de Planétologie et d’Astrophysique de Grenoble (IPAG)
A. Boccaletti, LESIA - Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique
A. Bohn, Sterrewacht Leiden
M. Bonnefoy, Institut de Planétologie et d’Astrophysique de Grenoble (IPAG)
H. Bonnet, European Southern Observatory
G. Bourdarot, Institut de Planétologie et d’Astrophysique de Grenoble (IPAG)
W. Brandner, Max Planck Institute for Astronomy
F. Cantalloube, Laboratoire d'Astrophysique de Marseille
P. Caselli, Max Planck Institute for Extraterrestrial Physics
B. Charnay, LESIA - Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique
G. Chauvin, Institut de Planétologie et d’Astrophysique de Grenoble (IPAG)

Author ORCID Identifier

Kimberly Ward-Duong: 0000-0002-4479-8291

Document Type

Article

Publication Date

10-1-2023

Publication Title

Astrophysical Journal

Abstract

Tension remains between the observed and modeled properties of substellar objects, but objects in binary orbits, with known dynamical masses, can provide a way forward. HD 72946 B is a recently imaged brown dwarf companion to a nearby, solar-type star. We achieve ∼100 μas relative astrometry of HD 72946 B in the K band using VLTI/GRAVITY, unprecedented for a benchmark brown dwarf. We fit an ensemble of measurements of the orbit using orbitize! and derive a strong dynamical mass constraint M B = 69.5 ± 0.5 M Jup assuming a strong prior on the host star mass M A = 0.97 ± 0.01 M ⊙ from an updated stellar analysis. We fit the spectrum of the companion to a grid of self-consistent BT-Settl-CIFIST model atmospheres, and perform atmospheric retrievals using petitRADTRANS. A dynamical mass prior only marginally influences the sampled distribution of effective temperature, but has a large influence on the surface gravity and radius, as expected. The dynamical mass alone does not strongly influence retrieved pressure-temperature or cloud parameters within our current retrieval setup. Independently of the cloud prescription and prior assumptions, we find agreement within ±2σ between the C/O of the host (0.52 ± 0.05) and brown dwarf (0.43-0.63), as expected from a molecular cloud collapse formation scenario, but our retrieved metallicities are implausibly high (0.6-0.8) in light of the excellent agreement of the data with the solar-abundance model grid. Future work on our retrieval framework will seek to resolve this tension. Additional study of low surface gravity objects is necessary to assess the influence of a dynamical mass prior on atmospheric analysis.

Volume

956

Issue

2

DOI

10.3847/1538-4357/acf761

ISSN

0004637X

Creative Commons License

Creative Commons Attribution 4.0 International License
This work is licensed under a Creative Commons Attribution 4.0 International License.

Rights

© 2023 The Authors

Comments

Archived as published.

Share

COinS
 
 

To view the content in your browser, please download Adobe Reader or, alternately,
you may Download the file to your hard drive.

NOTE: The latest versions of Adobe Reader do not support viewing PDF files within Firefox on Mac OS and if you are using a modern (Intel) Mac, there is no official plugin for viewing PDF files within the browser window.