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相关论文: The Early Merger that Made the Galaxy's Stellar Ha…

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Theoretical considerations and observational data support the idea that mergers were more frequent in the past. At high redshifts, violent interactions and mergers may be implicated in the origin of Lyman-break galaxies, sub-mm starbursts,…

天体物理学 · 物理学 2007-05-23 Joshua E. Barnes

We study the possibility that the Milky Way's cool stellar disc includes mergers with ancient stars. Galaxies are understood to form in a hierarchical manner, where smaller (proto-)galaxies merge into larger ones. Stars in galaxies, like…

星系天体物理 · 物理学 2022-07-27 Diane K. Feuillet , Sofia Feltzing , Christian Sahlholdt , Thomas Bensby

Stellar halos of galaxies retain crucial clues to their mass assembly history. It is in these galactic components that the remains of cannibalised galactic building blocks are deposited. For the case of the Milky Way, the opportunity to…

星系天体物理 · 物理学 2024-04-29 Danny Horta , Ricardo P. Schiavon

Theoretical considerations and observational data support the idea that mergers were more frequent in the past. At redshifts z = 2 to 5, violent interactions and mergers may be implicated by observations of Lyman-break galaxies, sub-mm…

天体物理学 · 物理学 2009-10-31 Joshua E. Barnes

The archaeological record of stars in the Milky Way opens a uniquely detailed window into the early formation and assembly of galaxies. Here we use 11,000 main-sequence turn-off stars with well-measured ages, [Fe/H], [$\alpha$/Fe], and…

Within the Cold Dark Matter scenario the hierarchical merging paradigm is the natural result to form massive galactic halos by the minor mergers of sub-halos and, by this, inherently their stellar halo. Although this must be also invoked…

宇宙学与河外天体物理 · 物理学 2015-05-27 Mykola Petrov , Gerhard Hensler

We present first results from a spectroscopic survey of 2000 F/G stars 0.5--5kpc from the Galactic plane, obtained with the 2dF facility on the AAT. These data show the mean rotation velocity of the thick disk about the Galactic center a…

天体物理学 · 物理学 2009-11-07 Gerard Gilmore , Rosemary F. G. Wyse , John E. Norris

If the favored hierarchical cosmological model is correct, then the Milky Way system should have accreted ~100-200 luminous satellite galaxies in the past \~12 Gyr. We model this process using a hybrid semi-analytic plus N-body approach…

天体物理学 · 物理学 2008-11-26 James S. Bullock , Kathryn V. Johnston

The standard cosmological model ($\Lambda$-CDM) predicts that galaxies are built through hierarchical assembly on cosmological timescales$^{1,2}$. The Milky Way, like other disc galaxies, underwent violent mergers and accretion of small…

The last 10-20 years has seen a profound shift in views of how the Galaxy's halo formed. The idea of a monolithic early collapse of a single system (Eggen, Lynden-Bell and Sandage 1962) has been challenged by observations at high redshift…

The prevailing model of galaxy formation proposes that galaxies like the Milky Way are built through a series of mergers with smaller galaxies over time. However, the exact details of the Milky Way's assembly history remain uncertain. In…

星系天体物理 · 物理学 2024-12-18 Lekshmi Thulasidharan , Elena D'Onghia , Robert Benjamin , Ronald Drimmel , Eloisa Poggio , Anna Queiroz

Current ideas on the formation of the Galaxy are reviewed. Many of the observed characteristics of our Milky Way System are consistent with a scenario in which the Galaxy formed inside out, with the inner part of it evolving by rapid…

天体物理学 · 物理学 2009-10-28 Sidney van den Bergh

A study of stellar ages of a sample from the Sloan Digital Sky Survey (SDSS) is presented. The results are consolidated with a set of globular clusters (GCs) and show that this stellar sample is composed by one dominant population of 10-12…

星系天体物理 · 物理学 2012-01-10 Paula Jofre

Near-field observations may provide tight constraints - i.e. "boundary conditions" - on any model of structure formation in the Universe. Detailed observational data have long been available for the Milky Way (e.g. Freeman $\&$…

星系天体物理 · 物理学 2015-06-16 Agostino Renda

Our Galaxy is thought to have undergone an active evolutionary history dominated by star formation, the accretion of cold gas, and, in particular, mergers up to 10 gigayear ago. The stellar halo reveals rich fossil evidence of these…

Reconstructing the mass assembly history of the Milky Way relies on obtaining detailed measurements of the properties of many stars in the Galaxy, especially in the stellar halo. One of the most constraining quantities is stellar age, as it…

星系天体物理 · 物理学 2024-06-11 Danny Horta , Yuxi , Lu , Melissa K. Ness , Mariangela Lisanti , Adrian M. Price-Whelan

The present day chemical and dynamical properties of the Milky Way bear the imprint of the Galaxy's formation and evolutionary history. One of the most enduring and critical debates surrounding Galactic evolution is that regarding the…

天体物理学 · 物理学 2009-11-07 Chris B. Brook , Daisuke Kawata , Brad K. Gibson , Chris Flynn

$Context$. The assembly history experienced by the Milky Way is currently being unveiled thanks to the data provided by the $Gaia$ mission. It is likely that the globular cluster system of our Galaxy has followed a similarly intricate…

星系天体物理 · 物理学 2019-09-25 Davide Massari , Helmer H. Koppelman , Amina Helmi

We have learned recently that the inner halo of the Milky Way contains a kinematically coherent component (Gaia-Enceladus) from a significant merger 10 Gyrs ago. By contrast the inner halo (defined to exclude the Magellanic Stream) contains…

星系天体物理 · 物理学 2019-03-20 Jeremy Mould

We study numerical simulations of satellite galaxy disruption in a potential resembling that of the Milky Way. Our goal is to assess whether a merger origin for the stellar halo would leave observable fossil structure in the phase-space…

天体物理学 · 物理学 2009-05-11 Amina Helmi , Simon D. M. White