Results 11 to 20 of about 29,619 (304)

The accretion origin of the Milky Way's stellar halo [PDF]

open access: yesThe Astrophysical Journal, 2008
We have used data from the Sloan Digital Sky Survey (SDSS) Data Release 5 to explore the overall structure and substructure of the stellar halo of the Milky Way using about 4 million color-selected main sequence turn-off stars. We fit oblate and triaxial
Adi Zolotov   +23 more
core   +7 more sources

Two Stellar Components in the Halo of the Milky Way [PDF]

open access: yesNature, 2007
The halo of the Milky Way provides unique elemental abundance and kinematic information on the first objects to form in the Universe, which can be used to tightly constrain models of galaxy formation and evolution. Although the halo was once considered a
A Dekel   +55 more
core   +5 more sources

The total stellar halo mass of the Milky Way [PDF]

open access: greenMonthly Notices of the Royal Astronomical Society, 2019
ABSTRACT We measure the total stellar halo luminosity using red giant branch (RGB) stars selected from Gaia data release 2. Using slices in magnitude, colour, and location on the sky, we decompose RGB stars belonging to the disc and halo by fitting two-dimensional Gaussians to the Galactic proper motion distributions.
Alis J. Deason   +2 more
openalex   +7 more sources

Stellar haloes in Milky-Way mass galaxies: From the inner to the outer haloes [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2014
We present a comprehensive study of the chemical properties of the stellar haloes of Milky-Way mass galaxies, analysing the transition between the inner to the outer haloes.
Beers, T.   +3 more
core   +3 more sources

Stellar Over-Densities in the Outer Halo of the Milky Way [PDF]

open access: bronzePublications of the Astronomical Society of Australia, 2010
AbstractThis study presents a tomographic survey of a subset of the outer halo (10–40 kpc) drawn from the Sloan Digital Sky Survey Data Release 6. Halo substructure on spatial scales of >3 degrees is revealed as an excess in the local density of sub-giant stars.
Stefan Keller
openalex   +6 more sources

The artemis simulations: stellar haloes of Milky Way-mass galaxies [PDF]

open access: greenMonthly Notices of the Royal Astronomical Society, 2020
ABSTRACT We introduce the Assembly of high-ResoluTion Eagle-simulations of MIlky Way-type galaxieS (artemis) simulations, a new set of 42 zoomed-in, high-resolution (baryon particle mass of $\approx 2\times 10^4 \, {\rm M}_{\odot }\, h^{-1}$), hydrodynamical simulations of galaxies residing in haloes of Milky Way mass, simulated with the
Andreea S. Font   +8 more
openalex   +7 more sources

The dual nature of the Milky Way stellar halo [PDF]

open access: bronzeProceedings of the International Astronomical Union, 2010
AbstractThe theory of the Milky Way formation, in the framework of the ΛCDM model, predicts galactic stellar halos to be built from multiple accretion events starting from the first structure to collapse in the Universe.Evidences in the past few decades have indicated that the Galactic halo consists of two overlapping structural components, an inner ...
A. Curir   +3 more
openalex   +2 more sources

The cold veil of the Milky Way stellar halo [PDF]

open access: bronzeMonthly Notices of the Royal Astronomical Society, 2012
15 pages, 12 figures.
Alis J. Deason   +9 more
openalex   +10 more sources

THE HERCULES SATELLITE: A STELLAR STREAM IN THE MILKY WAY HALO? [PDF]

open access: bronzeThe Astrophysical Journal, 2010
Conference proceedings of "A Universe of dwarf galaxies: Observations, Theories, Simulations" held in Lyon, France (June 14-18, 2010)
Nicolas F. Martin, Shoko Jin
openalex   +9 more sources

Mapping the milky way’s stellar halo with 2D data [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2023
ABSTRACT We propose a new method for measuring the spatial density distribution of the stellar halo of the Milky Way. Our method is based on a pairwise statistic of the distribution of stars in the sky, the angular two-point correlation function (ATPCF). The ATPCF utilizes two-dimensional data of stars only and is therefore immune to the
Anda Chen   +5 more
openaire   +2 more sources

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