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| Main Authors: | , , , , , , , |
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| Format: | Preprint |
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2026
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| Online Access: | https://arxiv.org/abs/2602.19755 |
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| _version_ | 1866917288506032128 |
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| author | McLachlan, Dan Ginski, Christian Byrne, Jake Lawlor, Chloe Campbell-White, Justyn Claes, Rik Ren, Bin Sierra, Anibal |
| author_facet | McLachlan, Dan Ginski, Christian Byrne, Jake Lawlor, Chloe Campbell-White, Justyn Claes, Rik Ren, Bin Sierra, Anibal |
| contents | This paper presents new data and analyses of the AT Pyx system, a disk-hosting young star located in a cometary globule in the Gum Nebula. This radiation-driven structure is an unusual environment for observations of planet formation and differs greatly from the low-mass star-forming regions disks are most commonly observed in. Aided by a collection of visual and spectroscopic data available for this system, this paper aims to infer the possibility of embedded planets existing within the disk and how the system's environment may affect its disk morphology. Using data from the VLT's instruments XSHOOTER, ESPRESSO and - most prominently - SPHERE along with data from ALMA, we make a variety of measurements (geometric, photometric and otherwise) to characterise the observed disk features and attributes such as spiral arms and eccentricity. Mapping of the velocity components is also undertaken using the ALMA gas line data to characterise disk orientation and determine the likelihood that the system is experiencing a late-stage infall event. The disk is found to be eccentric when deprojected. Under the assumption that the formation of a planet is wholly responsible for the primary and secondary spiral arms, we find the mass of such a planet can range between 0.004 and 3 Jupiter masses. Measurement of the velocities associated with nearby globule cloud material returns reasonable velocities for a late-stage infall event. We estimate far-ultraviolet field strength at AT Pyx's location to be low in comparison to other surveyed disks. We also find that AT Pyx is possibly a binary system. AT Pyx is the first disk within a cometary globule to be spatially resolved, and is now the first such disk to be investigated to this extent. The work of this paper could potentially be a first step into the further study of disks in the moderate-FUV environment of the Gum Nebula and its globules. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2602_19755 |
| institution | arXiv |
| publishDate | 2026 |
| record_format | arxiv |
| spellingShingle | Young system development in a cometary globule: An investigation into the eccentric disk around AT Pyx in terms of planet-formation and interaction with its surrounding environment McLachlan, Dan Ginski, Christian Byrne, Jake Lawlor, Chloe Campbell-White, Justyn Claes, Rik Ren, Bin Sierra, Anibal Earth and Planetary Astrophysics This paper presents new data and analyses of the AT Pyx system, a disk-hosting young star located in a cometary globule in the Gum Nebula. This radiation-driven structure is an unusual environment for observations of planet formation and differs greatly from the low-mass star-forming regions disks are most commonly observed in. Aided by a collection of visual and spectroscopic data available for this system, this paper aims to infer the possibility of embedded planets existing within the disk and how the system's environment may affect its disk morphology. Using data from the VLT's instruments XSHOOTER, ESPRESSO and - most prominently - SPHERE along with data from ALMA, we make a variety of measurements (geometric, photometric and otherwise) to characterise the observed disk features and attributes such as spiral arms and eccentricity. Mapping of the velocity components is also undertaken using the ALMA gas line data to characterise disk orientation and determine the likelihood that the system is experiencing a late-stage infall event. The disk is found to be eccentric when deprojected. Under the assumption that the formation of a planet is wholly responsible for the primary and secondary spiral arms, we find the mass of such a planet can range between 0.004 and 3 Jupiter masses. Measurement of the velocities associated with nearby globule cloud material returns reasonable velocities for a late-stage infall event. We estimate far-ultraviolet field strength at AT Pyx's location to be low in comparison to other surveyed disks. We also find that AT Pyx is possibly a binary system. AT Pyx is the first disk within a cometary globule to be spatially resolved, and is now the first such disk to be investigated to this extent. The work of this paper could potentially be a first step into the further study of disks in the moderate-FUV environment of the Gum Nebula and its globules. |
| title | Young system development in a cometary globule: An investigation into the eccentric disk around AT Pyx in terms of planet-formation and interaction with its surrounding environment |
| topic | Earth and Planetary Astrophysics |
| url | https://arxiv.org/abs/2602.19755 |