The contribution of Globular Clusters to the stellar halo using APOGEE and GAIA
2019 ◽
Vol 14
(S351)
◽
pp. 455-459
Keyword(s):
AbstractOver the last decade, much of the key questions in Galactic Archaeology have been asnwered by studying the Milky Way’s globular cluster (GC) system. Following on this, it has been shown that a substantial fraction of the Milky Way’s stellar halo field arises from GC dissolution. In this work, we make use of the latest data release fromn the APOGEE survey to study GC dissolution ratios in different spatial regions of the Galaxy. Our results will allow us to constrain many astrophysical questions, such as: the origin of N-Rich stars, the mass contribution from GCs to the stellar halo of the Galaxy, the origin of the Galactic GC system and the mass assembly of the Milky Way.
1988 ◽
Vol 126
◽
pp. 37-48
Keyword(s):
1983 ◽
Vol 100
◽
pp. 359-364
Keyword(s):
2017 ◽
Vol 26
(09)
◽
pp. 1730017
Keyword(s):
2019 ◽
Vol 14
(S351)
◽
pp. 420-421
Keyword(s):
2017 ◽
Vol 13
(S334)
◽
pp. 38-42
◽
Keyword(s):
2019 ◽
Vol 488
(1)
◽
pp. 1235-1247
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Keyword(s):
2019 ◽
Vol 491
(3)
◽
pp. 4012-4022
◽
Keyword(s):
2020 ◽
Vol 496
(1)
◽
pp. 638-648
◽
Keyword(s):
2020 ◽
Vol 500
(2)
◽
pp. 2514-2524
Keyword(s):
1964 ◽
Vol 20
◽
pp. 354-357