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| Main Authors: | , , , , , , , , , , , , , , , , , , , , , |
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| Format: | Preprint |
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2024
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| Online Access: | https://arxiv.org/abs/2407.16651 |
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| _version_ | 1866912426097639424 |
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| author | Sierra, Anibal Pérez, Laura M. Agurto-Gangas, Carolina Miley, James Zhang, Ke Pinilla, Paola Pascucci, Ilaria Trapman, Leon Kurtovic, Nicolas Vioque, Miguel Deng, Dingshan Anania, Rossella Carpenter, John Cieza, Lucas A. González-Ruilova, Camilo Hogerheijde, Michiel Kuznetsova, Aleksandra Rosotti, Giovanni P. Ruiz-Rodriguez, Dary A. Schwarz, Kamber Tabone, Benoît TorresVillanueva, Estephani E. |
| author_facet | Sierra, Anibal Pérez, Laura M. Agurto-Gangas, Carolina Miley, James Zhang, Ke Pinilla, Paola Pascucci, Ilaria Trapman, Leon Kurtovic, Nicolas Vioque, Miguel Deng, Dingshan Anania, Rossella Carpenter, John Cieza, Lucas A. González-Ruilova, Camilo Hogerheijde, Michiel Kuznetsova, Aleksandra Rosotti, Giovanni P. Ruiz-Rodriguez, Dary A. Schwarz, Kamber Tabone, Benoît TorresVillanueva, Estephani E. |
| contents | Detecting planet signatures in protoplanetary disks is fundamental to understanding how and where planets form. In this work, we report dust and gas observational hints of planet formation in the disk around 2MASS-J16120668-301027, as part of the ALMA Large Program "AGE-PRO: ALMA survey of Gas Evolution in Protoplanetary disks". The disk was imaged with the Atacama Large Millimeter/submillimeter Array (ALMA) at Band 6 (1.3 mm) in dust continuum emission and four molecular lines: $^{12}$CO(J=2-1), $^{13}$CO(J=2-1), C$^{18}$O(J=2-1), and H$_2$CO(J=3$_{(3,0)}$-2$_{(2,0)}$). Resolved observations of the dust continuum emission (angular resolution of $\sim 150$ mas, 20 au) show a ring-like structure with a peak at $0.57 ^{\prime \prime}$ (75 au), a deep gap with a minimum at 0.24$^{\prime \prime}$ (31 au), an inner disk, a bridge connecting the inner disk and the outer ring, along with a spiral arm structure, and a tentative detection (to $3σ$) of a compact emission at the center of the disk gap, with an estimated dust mass of $\sim 2.7-12.9$ Lunar masses. We also detected a kinematic kink (not coincident with any dust substructure) through several $^{12}$CO channel maps (angular resolution $\sim$ 200 mas, 30 au), located at a radius of $\sim 0.875^{\prime \prime}$ (115.6 au). After modeling the $^{12}$CO velocity rotation around the protostar, we identified a tentative rotating-like structure at the kink location with a geometry similar to that of the disk. We discuss potential explanations for the dust and gas substructures observed in the disk, and their potential connection to signatures of planet formation. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2407_16651 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Hints of planet formation signatures in a large-cavity disk studied in the AGE-PRO ALMA Large Program Sierra, Anibal Pérez, Laura M. Agurto-Gangas, Carolina Miley, James Zhang, Ke Pinilla, Paola Pascucci, Ilaria Trapman, Leon Kurtovic, Nicolas Vioque, Miguel Deng, Dingshan Anania, Rossella Carpenter, John Cieza, Lucas A. González-Ruilova, Camilo Hogerheijde, Michiel Kuznetsova, Aleksandra Rosotti, Giovanni P. Ruiz-Rodriguez, Dary A. Schwarz, Kamber Tabone, Benoît TorresVillanueva, Estephani E. Earth and Planetary Astrophysics Detecting planet signatures in protoplanetary disks is fundamental to understanding how and where planets form. In this work, we report dust and gas observational hints of planet formation in the disk around 2MASS-J16120668-301027, as part of the ALMA Large Program "AGE-PRO: ALMA survey of Gas Evolution in Protoplanetary disks". The disk was imaged with the Atacama Large Millimeter/submillimeter Array (ALMA) at Band 6 (1.3 mm) in dust continuum emission and four molecular lines: $^{12}$CO(J=2-1), $^{13}$CO(J=2-1), C$^{18}$O(J=2-1), and H$_2$CO(J=3$_{(3,0)}$-2$_{(2,0)}$). Resolved observations of the dust continuum emission (angular resolution of $\sim 150$ mas, 20 au) show a ring-like structure with a peak at $0.57 ^{\prime \prime}$ (75 au), a deep gap with a minimum at 0.24$^{\prime \prime}$ (31 au), an inner disk, a bridge connecting the inner disk and the outer ring, along with a spiral arm structure, and a tentative detection (to $3σ$) of a compact emission at the center of the disk gap, with an estimated dust mass of $\sim 2.7-12.9$ Lunar masses. We also detected a kinematic kink (not coincident with any dust substructure) through several $^{12}$CO channel maps (angular resolution $\sim$ 200 mas, 30 au), located at a radius of $\sim 0.875^{\prime \prime}$ (115.6 au). After modeling the $^{12}$CO velocity rotation around the protostar, we identified a tentative rotating-like structure at the kink location with a geometry similar to that of the disk. We discuss potential explanations for the dust and gas substructures observed in the disk, and their potential connection to signatures of planet formation. |
| title | Hints of planet formation signatures in a large-cavity disk studied in the AGE-PRO ALMA Large Program |
| topic | Earth and Planetary Astrophysics |
| url | https://arxiv.org/abs/2407.16651 |