Estimating the Initial Mass of the Gaia–Enceladus Dwarf Galaxy with a Chemical Evolution Model
The Astrophysical JournalThis work investigates the initial mass and chemical evolution history of the Gaia–Enceladus dwarf galaxy. We combine spectroscopic data from APOGEE with astrometric data from Gaia Data Release 3 to identify Gaia–Enceladus candidate stars via a machine ...
Olcay Plevne, Furkan Akbaba
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A census of AGB stars in the Milky Way and M31 subgroups of dwarf-spheroidal galaxies [PDF]
, 2004 F. Kirschbaum +5 more
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Is the Dust Obscuring Supernovae in Distant Galaxies the Same as Dust in the Milky Way?
, 1996 Adam G. Riess +2 more
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A New Milky Way Dwarf Galaxy in Ursa Major [PDF]
, 2005 Beth Willman +14 more
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A Catalog of Distance Determinations for 5 Million Stars in LAMOST DR10
The Astronomical JournalUsing the distance estimation method outlined in J. L. Carlin et al., a Bayesian approach specifically tailored for LAMOST data, we estimated distances for 7,450,303 spectra from 5,394,174 unique stars in the LAMOST DR10 low-resolution data set.
Chengqun Yang +5 more
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Non-association of a celestial gamma ray source with the new Milky Way satellite galaxy [PDF]
The newly discovered satellite galaxy located in the Milky Way galactic anti-center region is discussed along with the possibility that a nearby gamma ray source is associated with it.
Fichtel, C. E. +2 more
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Oxygen Abundances in the Milky Way Using X‐Ray Absorption Measurements toward Galaxy Clusters [PDF]
, 2006 W. H. Baumgartner, R. F. Mushotzky
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On the Origin of the 107 K Hot Emitting Gas in the Circumgalactic Medium of the Milky Way
The Astrophysical JournalThe presence of the ≈10 ^6 K gas in the circumgalactic medium of the Milky Way (MW) has been well established. However, the location and the origin of the newly discovered hot gas at “supervirial (SV)” temperatures of ≈10 ^7 K have been puzzling.
Mukesh Singh Bisht +2 more
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The spatial distribution of the Milky Way and Andromeda satellite galaxies [PDF]
, 2006 Manuel Metz, Pavel Kroupa, Helmut Jerjen
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Secular evolution of Milky Way-type galaxies
, 2017 The internal evolution of disk galaxies like the Milky Way are driven by non-axisymmetries (bars) and the implied angular momentum transfer of the matter; baryons are essentially driven inwards to build a more concentrated disk. This mass concentration may lead to the decoupling of a secondary bar, since the orbit precessing frequency is then much ...
openaire +3 more sources