Spectral analysis of two directly imaged benchmark L dwarf companions at the stellar-substellar boundary

We used multiple epochs of high-contrast imaging spectrophotometric observations to determine the atmospheric characteristics and thermal evolution of two previously detected benchmark L dwarf companions, HD 112863 B and HD 206505 B. We analyzed IRDIS and IFS data from VLT/SPHERE of each companion, both of which have dynamical masses near the stellar-substellar boundary. We compared each companion with empirical spectral standards, and constrained their physical properties through atmospheric model fits. From these analyses, we estimate that HD 112863 B is spectral type L3 ± 1 and that HD 206505 B is spectral type L2 ± 1. Using the BT-Settl atmospheric model grids, we found a bimodal solution for the atmospheric model fit of HD 112863 B where T eff = 1757 −36 +37 K or 2002 −24 +23 K and log g = 4.973 −0.063 +0.057 or 5.253 −0.033 +0.037 , while for HD 206505 B, T eff = 1754 −13 +13 K and log g = 4.919 −0.029 +0.031 . The results of a comparison of the bolometric luminosities of the companions with evolutionary models imply that both companions are likely above the hydrogen burning limit.

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Publication Details

Journal
Astronomy and Astrophysics
Published
2025-09-01
DOI
https://doi.org/10.1051/0004-6361/202555310
Citations
1
Primary Topic
Stellar, planetary, and galactic studies
Type
article
Field-Weighted Citation Impact
1.15

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Spectral analysis of two directly imaged benchmark L dwarf companions at the stellar-substellar boundary

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Stellar, planetary, and galactic studies
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article

Spectral analysis of two directly imaged benchmark L dwarf companions at the stellar-substellar boundary

J. Hagelberg, W. Ceva, D. Ségransan, Emily Rickman, Brendan P. Bowler, T. Forveille, Kyle Franson, Elisabeth C. Matthews, S. Udry, A. Vigan
article en
1 citations

Abstract

We used multiple epochs of high-contrast imaging spectrophotometric observations to determine the atmospheric characteristics and thermal evolution of two previously detected benchmark L dwarf companions, HD 112863 B and HD 206505 B. We analyzed IRDIS and IFS data from VLT/SPHERE of each companion, both of which have dynamical masses near the stellar-substellar boundary. We compared each companion with empirical spectral standards, and constrained their physical properties through atmospheric model fits. From these analyses, we estimate that HD 112863 B is spectral type L3 ± 1 and that HD 206505 B is spectral type L2 ± 1. Using the BT-Settl atmospheric model grids, we found a bimodal solution for the atmospheric model fit of HD 112863 B where T eff = 1757 −36 +37 K or 2002 −24 +23 K and log g = 4.973 −0.063 +0.057 or 5.253 −0.033 +0.037 , while for HD 206505 B, T eff = 1754 −13 +13 K and log g = 4.919 −0.029 +0.031 . The results of a comparison of the bolometric luminosities of the companions with evolutionary models imply that both companions are likely above the hydrogen burning limit.

Astronomy and AstrophysicsVol. 701
University of Geneva (CH), Centre National de la Recherche Scientifique (FR), Space Telescope Science Institute (US), University of California, Santa Barbara (US), Aix-Marseille Université (FR), Max Planck Institute for Astronomy (DE), The University of Texas at Austin (US), Université Grenoble Alpes (FR)
National Science Foundation, National Aeronautics and Space Administration, European Space Agency, Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung, Université de Genève
Openalex Percentile: Top 17%
Stellar, planetary, and galactic studies
1.15
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