New multi-zoom method for N-body simulations: application to galaxy growth by accretion
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Mass assembly of galaxiesDust and gas power spectrum in M 33 (HERM33ES)IMAGES IV: strong evolution of the oxygen abundance in gaseous phases of intermediate mass galaxies from z ~ 0.8IMAGES. II. A surprisingly low fraction of undisturbed rotating spiral disks at z ~ 0.6 The morpho-kinematical relation 6 Gyr agoIntegral field spectroscopy with SINFONI of VVDS galaxies. I. Galaxy dynamics and mass assembly at 1.2 < z < 1.6
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New multi-zoom method for N-body simulations: application to galaxy growth by accretion
description
article publié dans la revue scientifique Astronomy and Astrophysics
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im September 2005 veröffentlichter wissenschaftlicher Artikel
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scientific article published in Astronomy and Astrophysics
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wetenschappelijk artikel
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наукова стаття, опублікована у вересні 2005
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name
New multi-zoom method for N-body simulations: application to galaxy growth by accretion
@en
New multi-zoom method for N-body simulations: application to galaxy growth by accretion
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type
label
New multi-zoom method for N-body simulations: application to galaxy growth by accretion
@en
New multi-zoom method for N-body simulations: application to galaxy growth by accretion
@nl
prefLabel
New multi-zoom method for N-body simulations: application to galaxy growth by accretion
@en
New multi-zoom method for N-body simulations: application to galaxy growth by accretion
@nl
P2860
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New multi-zoom method for N-body simulations: application to galaxy growth by accretion
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B. Semelin
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10.1051/0004-6361:20042473
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P577
2005-09-13T00:00:00Z
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astro-ph/0506589
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2005A&A...441...55S