Revealing the structure and internal rotation of the Sagittarius dwarf spheroidal galaxy with gaia and machine learning

We present a detailed study of the internal structure and kinematics of the core of the Sagittarius dwarf spheroidal galaxy (Sgr). Using machine-learning techniques, we have combined the information provided by 3300 RR Lyrae stars, more than 2000 spectroscopically observed stars, and the Gaia second...

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Detalles Bibliográficos
Autor Principal: del Pino, Andrés (author)
Outros autores: Fardal, Mark A. (author), van der Marel, Roeland P. (author), Lokas, Ewa L. (author), Mateu, Cecilia (author), Sohn, Sangmo Tony (author)
Formato: article
Idioma:inglés
Publicado: 2021
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Acceso en liña:https://hdl.handle.net/20.500.12008/42199
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