The Milky Way Bar Potential Constrained by the Kinematics of SiO Maser Stars in BAaDE Survey
We introduce a novel method that utilizes the longitude–velocity ( l − v ) envelope to constrain the Milky Way (MW) bar potential. Previous work used the l − v diagram to explain the distribution of the observed high-velocity stars. We successfully reproduce their results but find that their method...
Gorde:
| Egile Nagusiak: | , , , , , , , |
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| Formatua: | Artigo |
| Hizkuntza: | Inglês |
| Argitaratua: |
IOP Publishing
2024-01-01
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| Saila: | The Astrophysical Journal |
| Gaiak: | |
| Sarrera elektronikoa: | https://doi.org/10.3847/1538-4357/ad834f |
| Etiketak: |
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