SiO v = 1 J = 5 → 4 Maser Emission from the Root of the “Water Fountain” Source W 43A

We report here the first mapping of SiO v = 1 J  = 5 → 4 maser emission toward the “water fountain” source W 43A in order to explore the central stellar system driving the collimated, bipolar, fast jet. The maser source has a systemic line-of-sight velocity consistent with that of CO J  = 2 → 1 emis...

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Detalhes bibliográficos

Principais autores:	Hiroshi Imai, Takeshi Hoshino, Daniel Tafoya, José F. Gómez, Jun-ichi Nakashima, Gabor Orosz
Formato:	Artigo
Idioma:	Inglês
Publicado em:	IOP Publishing 2025-01-01
coleção:	The Astrophysical Journal
Assuntos:	Circumstellar masers Stellar jets Stellar mass loss Common envelope evolution
Acesso em linha:	https://doi.org/10.3847/1538-4357/adde4e
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