Filamentary accretion cannot explain the orbital poles of the Milky Way satellites - Wikidata - awgldk - TriplyDB

Filamentary accretion cannot explain the orbital poles of the Milky Way satellites

Filamentary accretion cannot explain the orbital poles of the Milky Way satellites

http://www.wikidata.org/entity/Q58328575

about

Dwarf galaxy planes: the discovery of symmetric structures in the Local Group THE FAILURES OF THE STANDARD MODEL OF COSMOLOGY REQUIRE A NEW PARADIGM Co-orbiting satellite galaxy structures are still in conflict with the distribution of primordial dwarf galaxies What to expect from dynamical modelling of galactic haloes Alignments between galaxies, satellite systems and haloes A new spin on discs of satellite galaxies Stability of satellite planes in M31 II: effects of the dark subhalo population On the stability of satellite planes – I. Effects of mass, velocity, halo shape and alignment Understanding the internal dynamics of elliptical galaxies without non-baryonic dark matter A census of the expected properties of classical Milky Way dwarfs in Milgromian dynamics N-body simulations of the Carina dSph in MOND

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Filamentary accretion cannot explain the orbital poles of the Milky Way satellites

http://www.wikidata.org/entity/Q58328575

description

im Juni 2012 veröffentlichter wissenschaftlicher Artikel

@de

wetenschappelijk artikel

@nl

наукова стаття, опублікована в червні 2012

@uk

name

Filamentary accretion cannot explain the orbital poles of the Milky Way satellites

@en

Filamentary accretion cannot explain the orbital poles of the Milky Way satellites

@nl

type

label

Filamentary accretion cannot explain the orbital poles of the Milky Way satellites

@en

Filamentary accretion cannot explain the orbital poles of the Milky Way satellites

@nl

prefLabel

Filamentary accretion cannot explain the orbital poles of the Milky Way satellites

@en

Filamentary accretion cannot explain the orbital poles of the Milky Way satellites

@nl

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J.1365-2966.2012.21169.X

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Monthly Notices of the Royal Astronomical Society

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Filamentary accretion cannot explain the orbital poles of the Milky Way satellites

@en

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B. Famaey

http://www.w3.org/2001/XMLSchema#string

G. Angus

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G. Hensler

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K. S. de Boer

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M. S. Pawlowski

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P. Kroupa

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80–92

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scholarly article

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10.1111/J.1365-2966.2012.21169.X

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1

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424

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2012-06-12T00:00:00Z

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1204.6039

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2012MNRAS.424...80P

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