Considerations on the Origin of IRAS 19312+1950 Based on Long-term Maser Observations
IRAS source 19312+1950 (hereafter I19312) is an infrared point source with maser emissions of SiO, H _2 O, and OH molecules. Although initial observations suggested that I19312 might be an evolved star, its characteristics are not fully consistent with this classification. This study aims to further...
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| Main Authors: | Huan-Xue Feng, Jun-ichi Nakashima, D. Engels, S. Etoka, Jaeheon Kim, Yong Zhang, Jia-Yong Xie, Jian-Jie Qiu |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2025-01-01
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| Series: | The Astrophysical Journal |
| Subjects: | |
| Online Access: | https://doi.org/10.3847/1538-4357/adae09 |
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