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OH/IR stars in the inner Galactic bulge

Context. Stars on the asymptotic giant branch (AGB) play important roles in a number of astronomical contexts. To quantify these roles, it is necessary to establish the mass-loss characteristics of stars as they evolve up and beyond the AGB. Aims. We used an equidistant sample of 77 AGB stars in the...

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Autors principals: Olofsson H., Khouri T., Muller S., Unnikrishnan R., Groenewegen M. A. T., Blommaert J. A. D. L., De Beck E., Kastner J. H., Maercker M., Patel N., Ryde N., Sargent B. A., Srinivasan S., Vlemmings W. H. T.
Format: Artigo
Idioma:Inglês
Publicat: EDP Sciences 2026-06-01
Col·lecció:Astronomy & Astrophysics
Matèries:
stars: agb and post-agb
circumstellar matter
stars: mass-loss
Accés en línia:https://www.aanda.org/articles/aa/full_html/2026/06/aa60330-26/aa60330-26.html
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