A Multiwavelength View of ρ Oph. II. Disentangling the Variability of the Multistar Component C

Abstract We present a multiwavelength analysis of the star ρ Oph C, covering X-ray, optical, near-infrared (NIR), and radio observations to test for the presence of interferometrically detected cool star companions. The X-ray observations from Chandra, XMM-Newton, and NuSTAR show flare-like events lasting minutes or days in time and have spectral properties consistent with those of cooler stars instead of the primary magnetic B star. The NIR data are also consistent with the proposed trinary system properties due to the presence of CO bandheads. After removing the primary B star’s rotation, the optical data from TESS show a residual signal at the level of 0.8 mmag, matching the variations expected from cool stars in orbit around a bright B star. Finally, multiepoch radio data reveal that ρ Oph C exhibits significant large-scale flux variations that are atypical for a magnetic massive star. Taken as a whole, the multiepoch and -wavelength data present a consistent picture of ρ Oph C as a rare trinary system composed of a hot star and two cool stars.

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Publication Details

Journal
The Astrophysical Journal
Published
2026-10-28
DOI
https://doi.org/10.3847/1538-4357/aeac15
Primary Topic
Stellar, planetary, and galactic studies
Type
article
Field-Weighted Citation Impact
0.00

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article

A Multiwavelength View of ρ Oph. II. Disentangling the Variability of the Multistar Component C

Walter W. Golay, Pragati Pradhan, Sean J. Gunderson, Christiana Erba et al.
1 links
The Astrophysical Journal
Stellar, planetary, and galactic studies
article

A Multiwavelength View of ρ Oph. II. Disentangling the Variability of the Multistar Component C

Walter W. Golay, Pragati Pradhan, Sean J. Gunderson, Christiana Erba, John M. Cannon, Richard Ignace, A. Moreno, Felipe Navarete, Jackson Codd, David P. Huenemoerder
article en

Abstract

Abstract We present a multiwavelength analysis of the star ρ Oph C, covering X-ray, optical, near-infrared (NIR), and radio observations to test for the presence of interferometrically detected cool star companions. The X-ray observations from Chandra, XMM-Newton, and NuSTAR show flare-like events lasting minutes or days in time and have spectral properties consistent with those of cooler stars instead of the primary magnetic B star. The NIR data are also consistent with the proposed trinary system properties due to the presence of CO bandheads. After removing the primary B star’s rotation, the optical data from TESS show a residual signal at the level of 0.8 mmag, matching the variations expected from cool stars in orbit around a bright B star. Finally, multiepoch radio data reveal that ρ Oph C exhibits significant large-scale flux variations that are atypical for a magnetic massive star. Taken as a whole, the multiepoch and -wavelength data present a consistent picture of ρ Oph C as a rare trinary system composed of a hot star and two cool stars.

The Astrophysical JournalVol. 1011(1)
East Tennessee State University (US), University of Iowa (US), Space Telescope Science Institute (US), Center for Astrophysics Harvard & Smithsonian (US), Laboratório Nacional de Astrofísica (BR), Macalester College (US), Massachusetts Institute of Technology (US), California State University, Fresno (US), Embry–Riddle Aeronautical University (US)
Conselho Nacional de Desenvolvimento Científico e Tecnológico
Openalex Percentile: Top 14%
Stellar, planetary, and galactic studies
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