Results 41 to 50 of about 29,619 (304)
Stars made in outflows may populate the stellar halo of the Milky Way [PDF]
Monthly Notices of the Royal Astronomical Society, 2020 ABSTRACT We study stellar-halo formation using six Milky-Way-mass galaxies in FIRE-2 cosmological zoom simulations. We find that $5{-}40{{\ \rm per\ cent}}$ of the outer (50–300 kpc) stellar halo in each system consists of in-situ stars that were born in outflows from the main galaxy.
Andrew Wetzel +11 more
openaire +6 more sources
The Milky Way's stellar halo - lumpy or triaxial?
Journal of Physics: Conference Series, 2006 10 pages, 10 figs, to appear in proceedings of conference "Physics at the end of the Galactic Cosmic Ray Spectrum", Journal of Physics: Conf. series, eds. G.
Heidi Jo Newberg, Brian Yanny
openaire +3 more sources
Advanced Materials Interfaces, EarlyView., 2023 This review discusses the use of Surface‐Enhanced Raman Spectroscopy (SERS) combined with Artificial Intelligence (AI) for detecting antimicrobial resistance (AMR). Various SERS studies used with AI techniques, including machine learning and deep learning, are analyzed for their advantages and limitations.
Zakarya Al‐Shaebi +4 more
wiley +1 more source
The Milky Way stellar halo out to 40 kpc: squashed, broken but smooth [PDF]
Monthly Notices of the Royal Astronomical Society, 2011 13 pages, 12 figures.
Alis J. Deason +2 more
openalex +4 more sources
The galactic population of white dwarfs [PDF]
, 2009 Original paper can be found at: http://www.iop.org/EJ/conf DOI: 10.1088/1742-6596/172/1/012004 [16th European White Dwarfs Workshop]The contribution of white dwarfs of the different Galactic populations to the stellar content of our Galaxy is only poorly
Alcock C Allsman R A Alves D R +10 more
core +2 more sources
Formation ofin situstellar haloes in Milky Way-mass galaxies [PDF]
Monthly Notices of the Royal Astronomical Society, 2015 We study the formation of stellar haloes in three Milky Way-mass galaxies using cosmological smoothed particle hydrodynamics simulations, focusing on the subset of halo stars that form in situ, as opposed to those accreted from satellites. In situ stars in our simulations dominate the stellar halo out to 20 kpc and account for 30-40 per cent of its ...
Cooper, Andrew P. +4 more
openaire +4 more sources
The Nature of the Milky Way’s Stellar Halo Revealed by the Three Integrals of Motion [PDF]
The Astrophysical Journal, 2021 Abstract We developed a new selection method of halo stars in the phase-space distribution defined by the three integrals of motion in an axisymmetric Galactic potential (E, L z , I 3), where I 3 is the third integral of motion.
Daniela Carollo, Masashi Chiba
openaire +4 more sources
STELLAR VELOCITY DISPERSION AND ANISOTROPY OF THE MILKY WAY INNER HALO [PDF]
The Astrophysical Journal, 2015 15 pages, accepted to ...
Charles King III +3 more
openaire +3 more sources
Detection of Multiple Phase Space Overdensities of GSE Stars by Orbit Integration
The Astrophysical Journal, 2023 In N -body simulations, nearly radial mergers can form shell-like overdensities in the sky position and phase space ( r − v _r ) due to the combination of dynamical friction and tidal stripping.
Wenbo Wu +7 more
doaj +1 more source
The Outer Halo of the Milky Way as Probed by RR Lyr Variables from the Palomar Transient Facility [PDF]
, 2017 RR Lyr stars are ideal massless tracers that can be used to study the total mass and dark matter content of the outer halo of the Milky Way. This is because they are easy to find in the light curve databases of large stellar surveys and their distances ...
Bahnolzer, Sophianna +7 more
core +2 more sources