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Dynamical properties of a large young disk galaxy atz= 2.03

2008/06/16 by Lottie van Starkenburg, L. van Starkenburg, P. P. van der Werf +9 · 2 citations
Physics and Astronomy · #Astronomy #Astronomy and Astrophysical Research #Astrophysics #Context (archaeology) #Galaxies: Formation, Evolution, Phenomena #Galaxy #Galaxy formation and evolution #Geology #Physics #Redshift #Rest (music) #Rest frame #Star formation #Stellar, planetary, and galactic studies #astro-ph

paper · pdf · doi:10.1051/0004-6361:200809632

Accepted for publication in A&A, 15 pages, 14 figures

openalex publication_date 2008/06/16 · arxiv created 2008/06/20 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Context. The study of high redshift Tully-Fisher relations (TFRs) is limited by the use of long slit spectrographs, rest frame B band and star formation selected galaxies.

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