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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| Huvudupphov: | , , , , , , , |
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| Materialtyp: | Artigo |
| Språk: | Inglês |
| Utgiven: |
IOP Publishing
2025-01-01
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| Serie: | The Astrophysical Journal |
| Ämnen: | |
| Länkar: | https://doi.org/10.3847/1538-4357/adae09 |
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