Saved in:
| Main Authors: | , , , , , , , |
|---|---|
| Format: | Preprint |
| Published: |
2024
|
| Subjects: | |
| Online Access: | https://arxiv.org/abs/2407.13681 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
| _version_ | 1866911960867536896 |
|---|---|
| author | Martínez-Henares, Antonio Zhang, Qizhou Jiménez-Serra, Izaskun Martín-Pintado, Jesús Huélamo, Nuria Prasad, Sirina Moran, James Báez-Rubio, Alejandro |
| author_facet | Martínez-Henares, Antonio Zhang, Qizhou Jiménez-Serra, Izaskun Martín-Pintado, Jesús Huélamo, Nuria Prasad, Sirina Moran, James Báez-Rubio, Alejandro |
| contents | Jets and disk winds arise from materials with excess angular momentum ejected from the accretion disks in forming stars. How these structures are launched and how they impact the gas within the innermost regions of these objects remains poorly understood. MWC349A is a massive star that has a circumstellar disk which rotates in accord with Kepler's Law, with an ionized wind and a high-velocity jet launched from the disk surface. The strongly maser-amplified emission of hydrogen radio recombination lines (RRLs) observed toward this system provides a comprehensive picture of its ionized environment with exquisite detail. In this Letter, we present ALMA observations of the H26$α$ RRL and continuum emission obtained with the highest angular resolution ever used toward this source (beam of $\sim$0.02"). The maser RRL emission is resolved for the first time and clearly delineates the ionized disk, wind and jet. We analyzed the RRL data cubes with the 3D non-LTE radiative transfer model MORELI, confirming that the jet is poorly collimated. We found that the jet orientation is closer to the rotation axis of the system than derived from spatially unresolved data. This study confirms that hydrogen RRL masers are powerful probes of the physical structure and kinematics of the innermost ionized material around massive stars. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2407_13681 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Imaging the jet of MWC 349A with resolved Radio Recombination Line emission from ALMA Martínez-Henares, Antonio Zhang, Qizhou Jiménez-Serra, Izaskun Martín-Pintado, Jesús Huélamo, Nuria Prasad, Sirina Moran, James Báez-Rubio, Alejandro Solar and Stellar Astrophysics Astrophysics of Galaxies High Energy Astrophysical Phenomena Jets and disk winds arise from materials with excess angular momentum ejected from the accretion disks in forming stars. How these structures are launched and how they impact the gas within the innermost regions of these objects remains poorly understood. MWC349A is a massive star that has a circumstellar disk which rotates in accord with Kepler's Law, with an ionized wind and a high-velocity jet launched from the disk surface. The strongly maser-amplified emission of hydrogen radio recombination lines (RRLs) observed toward this system provides a comprehensive picture of its ionized environment with exquisite detail. In this Letter, we present ALMA observations of the H26$α$ RRL and continuum emission obtained with the highest angular resolution ever used toward this source (beam of $\sim$0.02"). The maser RRL emission is resolved for the first time and clearly delineates the ionized disk, wind and jet. We analyzed the RRL data cubes with the 3D non-LTE radiative transfer model MORELI, confirming that the jet is poorly collimated. We found that the jet orientation is closer to the rotation axis of the system than derived from spatially unresolved data. This study confirms that hydrogen RRL masers are powerful probes of the physical structure and kinematics of the innermost ionized material around massive stars. |
| title | Imaging the jet of MWC 349A with resolved Radio Recombination Line emission from ALMA |
| topic | Solar and Stellar Astrophysics Astrophysics of Galaxies High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2407.13681 |