Unveiling the infrared excess of SIPS J2045–6332: evidence for a young stellar object with potential low-mass companion

ABSTRACT The Disc Detective project, a citizen science initiative, aims to identify circumstellar discs around stars by detecting objects with infrared (IR) excess using data from the Wide-field Infrared Survey Explorer (WISE). In this study, we investigate SIPS J2045–6332, a potential brown dwarf with significant IR excess in WISE and Two Micron All Sky Survey (2MASS) bands, initially identified by project volunteers. Despite early indicators of a circumstellar disc, discrepancies between observed brightness and expected spectral energy distribution (SED) models suggested unusual properties. To explore potential explanations, we created SED templates for spectral types M9 to L4 and compared them with SIPS J2045–6332’s photometric data, revealing an excess brightness that points to either an unresolved low-mass companion or a young, inflated primary star. Further analysis of IR spectral features and surface gravity indicators supports a youthful classification, estimating the object’s age at 26–200 million years. Observations also suggest the presence of a mid L-type companion at a projected distance of 6.7 au. This study highlights SIPS J2045–6332 as an intriguing system with unique IR characteristics and recommends follow-up observations with high-resolution telescopes to confirm the companion hypothesis and further characterize the system.

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Publication Details

Journal
Monthly Notices of the Royal Astronomical Society
Published
2025-02-28
DOI
https://doi.org/10.1093/mnras/staf360
Citations
1
Primary Topic
Stellar, planetary, and galactic studies
Type
article
Field-Weighted Citation Impact
1.15
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article

Unveiling the infrared excess of SIPS J2045–6332: evidence for a young stellar object with potential low-mass companion

Adam C. Schneider, Jacqueline K. Faherty, Dan Caselden, Michiharu Hyogo et al.
1 citations
Monthly Notices of the Royal Astronomical Society
Stellar, planetary, and galactic studies
1.15
article

Unveiling the infrared excess of SIPS J2045–6332: evidence for a young stellar object with potential low-mass companion

Adam C. Schneider, Jacqueline K. Faherty, Dan Caselden, Michiharu Hyogo, Hugo A. Durantini Luca, Adam J. Burgasser, S. L. Casewell, J. Davy Kirkpatrick, Thomas P. Bickle, Federico Marocco, Steven M. Silverberg, Jonathan Gagné, Austin Rothermich, Sergio Dieterich, C. M. Lisse, Aaron Meisner, Daniella C. Bardalez Gagliuffi, Marc J. Kuchner, Joseph R. Biggs
article en
1 citations

Abstract

ABSTRACT The Disc Detective project, a citizen science initiative, aims to identify circumstellar discs around stars by detecting objects with infrared (IR) excess using data from the Wide-field Infrared Survey Explorer (WISE). In this study, we investigate SIPS J2045–6332, a potential brown dwarf with significant IR excess in WISE and Two Micron All Sky Survey (2MASS) bands, initially identified by project volunteers. Despite early indicators of a circumstellar disc, discrepancies between observed brightness and expected spectral energy distribution (SED) models suggested unusual properties. To explore potential explanations, we created SED templates for spectral types M9 to L4 and compared them with SIPS J2045–6332’s photometric data, revealing an excess brightness that points to either an unresolved low-mass companion or a young, inflated primary star. Further analysis of IR spectral features and surface gravity indicators supports a youthful classification, estimating the object’s age at 26–200 million years. Observations also suggest the presence of a mid L-type companion at a projected distance of 6.7 au. This study highlights SIPS J2045–6332 as an intriguing system with unique IR characteristics and recommends follow-up observations with high-resolution telescopes to confirm the companion hypothesis and further characterize the system.

Monthly Notices of the Royal Astronomical SocietyVol. 538(2)
The Graduate Center, CUNY (US), California Institute of Technology (US), Goddard Space Flight Center (US), American Museum of Natural History (US), Smithsonian Astrophysical Observatory (US), University of Leicester (GB), City University of New York (US), Amherst College (US), The Open University (GB), Espace pour la vie (CA), Johns Hopkins University Applied Physics Laboratory (US), University of California San Diego (US), Rio Tinto (Canada) (CA), Université Bourgogne Franche-Comté (FR), NSF NOIRLab (US), United States Naval Observatory (US), Detectogen (United States) (US), Backyard Brains (United States) (US), Infrared Processing and Analysis Center (US), Fundacion Allende (AR), Université de Montréal (CA)
Openalex Percentile: Top 21%
Stellar, planetary, and galactic studies
1.15
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