Searching for Protoplanets around MWC 758 and MWC 480 in Br-γ Using Kernel Phase and SCExAO/CHARIS Article Swipe
Alexander Chaushev
,
Steph Sallum
,
Julien Lozi
,
Jeffrey Chilcote
,
Tyler D. Groff
,
Olivier Guyon
,
N. Jeremy Kasdin
,
Barnaby Norris
,
Andrew Skemer
·
YOU?
·
· 2024
· Open Access
·
· DOI: https://doi.org/10.3847/1538-3881/ad528d
YOU?
·
· 2024
· Open Access
·
· DOI: https://doi.org/10.3847/1538-3881/ad528d
Discovering new actively accreting protoplanets is crucial to answering open questions about planet formation. However, identifying such planets at orbital distances where they are expected to be abundant is extremely challenging, both due to the technical requirements and large distances to star-forming regions. Here we use the kernel phase interferometry (KPI) technique to search for companions around the ∼6 and ∼8 Myr old Herbig Ae stars MWC 758 and MWC 480. KPI is a data analysis technique that is sensitive to moderate asymmetries, arising from, e.g., a circumstellar disk or companions with contrasts of up to 6–8 mag, at separations down to and even below the classical Rayleigh diffraction limit (∼1.2 λ / D ). Using the high-spectral-resolution K -band mode of the SCExAO/CHARIS integral field spectrograph, we search for both excess Br- γ line emission and continuum emission from companions around MWC 480 and MWC 758. We are able to set limits on the presence of rapidly accreting protoplanets and brown dwarfs between 4 and 16 au, well interior to those of previous studies. In Br- γ , we set limits on excess line emission equivalent to accretion rates ranging from to . Our achievable contrasts demonstrate that KPI using SCExAO/CHARIS is a promising technique to search for giant accreting protoplanets at smaller separations compared to conventional imaging.
Related Topics
Concepts
Integral field spectrograph
Physics
Protoplanet
Astrophysics
Stars
Algorithm
Spectrograph
Computer science
Astronomy
Spectral line
Protoplanetary disk
Metadata
- Type
- article
- Language
- en
- Landing Page
- http://doi.org/10.3847/1538-3881/ad528d
- OA Status
- gold
- Cited By
- 2
- References
- 70
- Related Works
- 10
- OpenAlex ID
- https://openalex.org/W4400558857
All OpenAlex metadata
Raw OpenAlex JSON
- OpenAlex ID
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https://openalex.org/W4400558857Canonical identifier for this work in OpenAlex
- DOI
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https://doi.org/10.3847/1538-3881/ad528dDigital Object Identifier
- Title
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Searching for Protoplanets around MWC 758 and MWC 480 in Br-γ Using Kernel Phase and SCExAO/CHARISWork title
- Type
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articleOpenAlex work type
- Language
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enPrimary language
- Publication year
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2024Year of publication
- Publication date
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2024-07-11Full publication date if available
- Authors
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Alexander Chaushev, Steph Sallum, Julien Lozi, Jeffrey Chilcote, Tyler D. Groff, Olivier Guyon, N. Jeremy Kasdin, Barnaby Norris, Andrew SkemerList of authors in order
- Landing page
-
https://doi.org/10.3847/1538-3881/ad528dPublisher landing page
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YesWhether a free full text is available
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goldOpen access status per OpenAlex
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https://doi.org/10.3847/1538-3881/ad528dDirect OA link when available
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Integral field spectrograph, Physics, Protoplanet, Astrophysics, Stars, Algorithm, Spectrograph, Computer science, Astronomy, Spectral line, Protoplanetary diskTop concepts (fields/topics) attached by OpenAlex
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2Total citation count in OpenAlex
- Citations by year (recent)
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2025: 1, 2024: 1Per-year citation counts (last 5 years)
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10Other works algorithmically related by OpenAlex
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