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pro vyhledávání: '"Barbillon, M."'
Autor:
Barbillon, M., Recio-Blanco, A., Poggio, E., Palicio, P. A., Spitoni, E., de Laverny, P., Cescutti, G.
The distribution of chemical elements in the Galactic disc can reveal fundamental clues on the physical processes that led to the current configuration of our Galaxy. We map chemical azimuthal variations in the disc using individual stellar chemical
Externí odkaz:
http://arxiv.org/abs/2411.10007
Autor:
Spitoni, E., Cescutti, G., Recio-Blanco, A., Minchev, I., Poggio, E., Palicio, P. A., Matteucci, F., Peirani, S., Barbillon, M., Vasini, A.
Publikováno v:
A&A 680, A85 (2023)
According to observations and numerical simulations, the Milky Way could exhibit several spiral arm modes with multiple pattern speeds, wherein the slower patterns are located at larger Galactocentric distances. Our aim is to quantify the effects of
Externí odkaz:
http://arxiv.org/abs/2310.11504