ALMASOP. A Rotating Feature Rich in Complex Organic Molecules in a Protostellar Core
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2025
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| author | Hsu, Shih-Ying Lee, Chin-Fei Johnstone, Doug Liu, Sheng-Yuan Liu, Tie Bronfman, Leonardo Chen, Huei-Ru Vivien Dutta, Somnath Eden, David J. Hirano, Naomi Juvela, Mika Kim, Kee-Tae Kuan, Yi-Jehng Kwon, Woojin Lee, Chang Won Lee, Jeong-Eun Li, Shanghuo Lin, Sheng-Jun Liu, Chun-Fan Liu, Xunchuan López-Vázquez, J. A. Luo, Qiuyi Rawlings, Mark G. Sahu, Dipen Sanhueza, Patricio Shang, Hsien Tatematsu, Kenichi Yang, Yao-Lun |
| author_facet | Hsu, Shih-Ying Lee, Chin-Fei Johnstone, Doug Liu, Sheng-Yuan Liu, Tie Bronfman, Leonardo Chen, Huei-Ru Vivien Dutta, Somnath Eden, David J. Hirano, Naomi Juvela, Mika Kim, Kee-Tae Kuan, Yi-Jehng Kwon, Woojin Lee, Chang Won Lee, Jeong-Eun Li, Shanghuo Lin, Sheng-Jun Liu, Chun-Fan Liu, Xunchuan López-Vázquez, J. A. Luo, Qiuyi Rawlings, Mark G. Sahu, Dipen Sanhueza, Patricio Shang, Hsien Tatematsu, Kenichi Yang, Yao-Lun |
| contents | Interstellar complex organic molecules (COMs) in solar-like young stellar objects (YSOs), particularly within protostellar disks, are of significant interest due to their potential connection to prebiotic chemistry in emerging planetary systems. We report the discovery of a rotating feature enriched in COMs, including CH3OH, CH3CHO, and NH2CHO, in the protostellar core G192.12-11.10. By constructing a YSO model, we find that the COM-rich feature is likely located within or near the boundary of the Keplerian disk. The image synthesis results suggest that additional heating mechanisms leading to a warm ring or a warm inner disk are required to reproduce the observed emission. We discuss possible origins of the COM-rich feature, particularly accretion shocks as a plausible cause for a warm ring. Additionally, molecules such as C18O, H2CO, DCS, H2S, and OCS exhibit distinct behavior compared to CH3OH, indicating a range of physical and chemical conditions within the region. The observed kinematics of H2S and OCS suggest that OCS resides in regions closer to the central protostar than H2S, consistent with previous experimental studies. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2506_15140 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | ALMASOP. A Rotating Feature Rich in Complex Organic Molecules in a Protostellar Core Hsu, Shih-Ying Lee, Chin-Fei Johnstone, Doug Liu, Sheng-Yuan Liu, Tie Bronfman, Leonardo Chen, Huei-Ru Vivien Dutta, Somnath Eden, David J. Hirano, Naomi Juvela, Mika Kim, Kee-Tae Kuan, Yi-Jehng Kwon, Woojin Lee, Chang Won Lee, Jeong-Eun Li, Shanghuo Lin, Sheng-Jun Liu, Chun-Fan Liu, Xunchuan López-Vázquez, J. A. Luo, Qiuyi Rawlings, Mark G. Sahu, Dipen Sanhueza, Patricio Shang, Hsien Tatematsu, Kenichi Yang, Yao-Lun Astrophysics of Galaxies Solar and Stellar Astrophysics Interstellar complex organic molecules (COMs) in solar-like young stellar objects (YSOs), particularly within protostellar disks, are of significant interest due to their potential connection to prebiotic chemistry in emerging planetary systems. We report the discovery of a rotating feature enriched in COMs, including CH3OH, CH3CHO, and NH2CHO, in the protostellar core G192.12-11.10. By constructing a YSO model, we find that the COM-rich feature is likely located within or near the boundary of the Keplerian disk. The image synthesis results suggest that additional heating mechanisms leading to a warm ring or a warm inner disk are required to reproduce the observed emission. We discuss possible origins of the COM-rich feature, particularly accretion shocks as a plausible cause for a warm ring. Additionally, molecules such as C18O, H2CO, DCS, H2S, and OCS exhibit distinct behavior compared to CH3OH, indicating a range of physical and chemical conditions within the region. The observed kinematics of H2S and OCS suggest that OCS resides in regions closer to the central protostar than H2S, consistent with previous experimental studies. |
| title | ALMASOP. A Rotating Feature Rich in Complex Organic Molecules in a Protostellar Core |
| topic | Astrophysics of Galaxies Solar and Stellar Astrophysics |
| url | https://arxiv.org/abs/2506.15140 |