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Towards sub-kpc scale kinematics of molecular and ionized gas of star-forming galaxies at z similar to 1

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    SYSNO ASEP0539811
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JČlánek ve WOS
    TitleTowards sub-kpc scale kinematics of molecular and ionized gas of star-forming galaxies at z similar to 1
    Author(s) Girard, M. (CH)
    Number of authors7
    Article numberA91
    Source TitleAstronomy & Astrophysics. - : EDP Sciences - ISSN 0004-6361
    Roč. 631, October (2019)
    Number of pages10 s.
    Publication formOnline - E
    Languageeng - English
    CountryFR - France
    Keywordsgalaxies ; high-redshift ; kinematics and dynamics
    Subject RIVBN - Astronomy, Celestial Mechanics, Astrophysics
    OECD categoryAstronomy (including astrophysics,space science)
    Research InfrastructureEU-ARC.CZ - 90067 - Astronomický ústav AV ČR, v. v. i.
    Method of publishingOpen access
    UT WOS000515093500001
    EID SCOPUS85074574217
    DOI10.1051/0004-6361/201935896
    AnnotationWe compare the molecular and ionized gas kinematics of two strongly lensed galaxies at z similar to 1 that lie on the main sequence at this redshift. The observations were made with ALMA and MUSE, respectively. We derive the CO and [OII] rotation curves and dispersion profiles of these two galaxies. We find a difference between the observed molecular and ionized gas rotation curves for one of the two galaxies, the Cosmic Snake, for which we obtain a spatial resolution of a few hundred parsec along the major axis. The rotation curve of the molecular gas is steeper than the rotation curve of the ionized gas. In the second galaxy, A521, the molecular and ionized gas rotation curves are consistent, but the spatial resolution is only a few kiloparsec on the major axis. Using simulations, we investigate the effect of the thickness of the gas disk and effective radius on the observed rotation curves and find that a more extended and thicker disk smoothens the curve.
    WorkplaceAstronomical Institute
    ContactRadka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326
    Year of Publishing2021
    Electronic addresshttps://doi.org/10.1051/0004-6361/201935896
Number of the records: 1  

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