Young stars discovered in dwarf spheroidal galaxies confirm their recent infall into the Milky way

Fuente: arXiv
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Main Authors: Hammer, Francois, Bonifacio, Piercarlo, Caffau, Elisabetta, Yang, Yanbin, Arenou, Frederic, Babusiaux, Carine, Spite, Monique, Francois, Patrick, Gomez, Ana, Katz, David, Monaco, Lorenzo, Pawlowski, Marcel, Wang, Jianling
Format: Preprint
Published: 2025
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author Hammer, Francois
Bonifacio, Piercarlo
Caffau, Elisabetta
Yang, Yanbin
Arenou, Frederic
Babusiaux, Carine
Spite, Monique
Francois, Patrick
Gomez, Ana
Katz, David
Monaco, Lorenzo
Pawlowski, Marcel
Wang, Jianling
author_facet Hammer, Francois
Bonifacio, Piercarlo
Caffau, Elisabetta
Yang, Yanbin
Arenou, Frederic
Babusiaux, Carine
Spite, Monique
Francois, Patrick
Gomez, Ana
Katz, David
Monaco, Lorenzo
Pawlowski, Marcel
Wang, Jianling
contents Recent observations from the ESA Gaia satellite and with the ESO VLT, have identified the presence of a population of young, 0.5 to 2 Gyr old, stars in the halo and in dwarf spheroidal galaxies surrounding the Milky Way. It suggests that MW dwarf galaxies, currently devoid of gas, had, until recent times, enough gas to sustain a burst of star formation. The recent loss of gas coincides with their arrival in the vicinity of the Milky Way, in agreement with orbital predictions from Gaia that indicate that most dwarf galaxies reached the Milky Way halo less than 3 Gyr years ago. This completely changes the interpretation of their dynamics, mass, and dark matter content.
format Preprint
id arxiv_https___arxiv_org_abs_2505_11587
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Young stars discovered in dwarf spheroidal galaxies confirm their recent infall into the Milky way
Hammer, Francois
Bonifacio, Piercarlo
Caffau, Elisabetta
Yang, Yanbin
Arenou, Frederic
Babusiaux, Carine
Spite, Monique
Francois, Patrick
Gomez, Ana
Katz, David
Monaco, Lorenzo
Pawlowski, Marcel
Wang, Jianling
Astrophysics of Galaxies
Recent observations from the ESA Gaia satellite and with the ESO VLT, have identified the presence of a population of young, 0.5 to 2 Gyr old, stars in the halo and in dwarf spheroidal galaxies surrounding the Milky Way. It suggests that MW dwarf galaxies, currently devoid of gas, had, until recent times, enough gas to sustain a burst of star formation. The recent loss of gas coincides with their arrival in the vicinity of the Milky Way, in agreement with orbital predictions from Gaia that indicate that most dwarf galaxies reached the Milky Way halo less than 3 Gyr years ago. This completely changes the interpretation of their dynamics, mass, and dark matter content.
title Young stars discovered in dwarf spheroidal galaxies confirm their recent infall into the Milky way
topic Astrophysics of Galaxies
url https://arxiv.org/abs/2505.11587