Small and Large Dust Cavities in Disks around Mid-M Stars in Taurus Article Swipe
YOU?
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· 2024
· Open Access
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· DOI: https://doi.org/10.3847/1538-4357/ad2e94
High angular resolution imaging by Atacama Large Millimeter/submillimeter Array (ALMA) has revealed the near universality and diversity of substructures in protoplanetary disks. However, disks around M-type pre-main-sequence stars are still poorly sampled, despite the prevalence of M dwarfs in the Galaxy. Here we present high-resolution (∼50 mas, 8 au) ALMA Band 6 observations of six disks around mid-M stars in Taurus. We detect dust continuum emission in all six disks, 12 CO in five disks, and 13 CO line in two disks. The size ratios between gas and dust disks range from 1.6 to 5.1. The ratio of about 5 for 2M0436 and 2M0450 indicates efficient dust radial drift. Four disks show rings and cavities, and two disks are smooth. The cavity sizes occupy a wide range: 60 au for 2M0412, and ∼10 au for 2M0434, 2M0436, and 2M0508. Detailed visibility modeling indicates that small cavities of 1.7 and 5.7 au may hide in the two smooth disks 2M0450 and CIDA 12. We perform radiative transfer fitting of the infrared spectral energy distributions to constrain the cavity sizes, finding that micron-sized dust grains may have smaller cavities than millimeter grains. Planet–disk interactions are the preferred explanation to produce the large 60 au cavity, while other physics could be responsible for the three ∼10 au cavities under current observations and theories. Currently, disks around mid- to late M stars in Taurus show a higher detection frequency of cavities than earlier-type stars, although a more complete sample is needed to evaluate any dependence of substructure on stellar mass.
Related Topics
- Type
- article
- Language
- en
- Landing Page
- https://doi.org/10.3847/1538-4357/ad2e94
- OA Status
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- Cited By
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- OpenAlex ID
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Raw OpenAlex JSON
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https://openalex.org/W4395455905Canonical identifier for this work in OpenAlex
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https://doi.org/10.3847/1538-4357/ad2e94Digital Object Identifier
- Title
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Small and Large Dust Cavities in Disks around Mid-M Stars in TaurusWork title
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articleOpenAlex work type
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enPrimary language
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2024Year of publication
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2024-04-25Full publication date if available
- Authors
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Yangfan Shi, Feng Long, Gregory J. Herczeg, D. Harsono, Yao Liu, Paola Pinilla, Enrico Ragusa, Doug Johnstone, Xue‐Ning Bai, Ilaria Pascucci, C. F. Manara, Gijs D. Mulders, Lucas A. CiezaList of authors in order
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https://doi.org/10.3847/1538-4357/ad2e94Publisher 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/10.3847/1538-4357/ad2e94Direct OA link when available
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Stars, Astrophysics, Astronomy, Astrobiology, PhysicsTop concepts (fields/topics) attached by OpenAlex
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11Total citation count in OpenAlex
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2025: 10, 2024: 1Per-year citation counts (last 5 years)
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199Number of works referenced by this work
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10Other works algorithmically related by OpenAlex
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| primary_location.raw_source_name | The Astrophysical Journal |
| primary_location.landing_page_url | https://doi.org/10.3847/1538-4357/ad2e94 |
| publication_date | 2024-04-25 |
| publication_year | 2024 |
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