Serendipitous observation of a white dwarf companion to a <i>JWST</i>/MIRI coronagraphic calibrator

ABSTRACT We present the unplanned detection of a white dwarf companion to the star HD 218261 in mid-infrared (10–16 $\mu$m) observations with JWST/MIRI. This star was observed as a calibrator for coronagraphic observations of the exoplanet host HR 8799. HD 218261 B has only previously been detected by Gaia, and only in visible light. We confidently detect the companion in the mid-infrared, where it is less luminous than the primary by a factor of ${\sim} 10^4$. The visible and mid-infrared photometry are consistent with a white dwarf of $T_\text{eff}\approx 10000$ K, $M\approx 0.8~\mathrm{ M}_\odot$, though observation of its optical spectrum is required to precisely constrain its physical parameters. These results demonstrate that precise mid-infrared photometry of white dwarf companions to bright stars can be obtained with MIRI, opening up new possibilities for studying white dwarfs in close binaries.

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Journal
Monthly Notices of the Royal Astronomical Society Letters
Published
2024-11-04
DOI
https://doi.org/10.1093/mnrasl/slae106
Citations
1
Primary Topic
Stellar, planetary, and galactic studies
Type
article
Field-Weighted Citation Impact
0.33

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article

Serendipitous observation of a white dwarf companion to a JWST/MIRI coronagraphic calibrator

Mary Anne Limbach, Alexander Venner, Mathilde Mâlin, Logan Pearce et al.
1 citations
Monthly Notices of the Royal Astronomical Society Letters
Stellar, planetary, and galactic studies
0.33
article

Serendipitous observation of a white dwarf companion to a JWST/MIRI coronagraphic calibrator

Mary Anne Limbach, Alexander Venner, Mathilde Mâlin, Logan Pearce, A. Boccaletti, Simon Blouin
article en
1 citations

Abstract

ABSTRACT We present the unplanned detection of a white dwarf companion to the star HD 218261 in mid-infrared (10–16 $\mu$m) observations with JWST/MIRI. This star was observed as a calibrator for coronagraphic observations of the exoplanet host HR 8799. HD 218261 B has only previously been detected by Gaia, and only in visible light. We confidently detect the companion in the mid-infrared, where it is less luminous than the primary by a factor of ${\sim} 10^4$. The visible and mid-infrared photometry are consistent with a white dwarf of $T_\text{eff}\approx 10000$ K, $M\approx 0.8~\mathrm{ M}_\odot$, though observation of its optical spectrum is required to precisely constrain its physical parameters. These results demonstrate that precise mid-infrared photometry of white dwarf companions to bright stars can be obtained with MIRI, opening up new possibilities for studying white dwarfs in close binaries.

Monthly Notices of the Royal Astronomical Society LettersVol. 536(1)
Centre National de la Recherche Scientifique (FR), Space Telescope Science Institute (US), Johns Hopkins University (US), Délégation Paris 7 (FR), University of Southern Queensland (AU), Université Paris Cité (FR), University of Victoria (CA), Université Paris Sciences et Lettres (FR), University of Michigan (US), Johns Hopkins Medicine (US), Sorbonne Université (FR), Sorbonne Paris Cité (FR), Laboratoire d’études spatiales et d’instrumentation en astrophysique (FR), Astronomy Australia (AU), University of Baltimore (US)
National Aeronautics and Space Administration, California Institute of Technology, University of Michigan, Space Telescope Science Institute, European Space Agency, Swinburne University of Technology, Jet Propulsion Laboratory, University of California, Los Angeles
Openalex Percentile: Top 33%
Stellar, planetary, and galactic studies
0.33
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