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Mapping the working of environmental effects in A963

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F20%3A00535571" target="_blank" >RIV/67985815:_____/20:00535571 - isvavai.cz</a>

  • Result on the web

    <a href="https://doi.org/10.1051/0004-6361/202037803" target="_blank" >https://doi.org/10.1051/0004-6361/202037803</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1051/0004-6361/202037803" target="_blank" >10.1051/0004-6361/202037803</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Mapping the working of environmental effects in A963

  • Original language description

    We qualitatively assess and map the relative contribution of pre-processing and cluster related processes to the build-up of A963, a massive cluster at z=0.2 showing an unusually high fraction of star forming galaxies in its interior. We report the first tentative observations at 21 cm of ongoing ram-pressure stripping at z=0.2, as well as observed inflow of low-entropy gas into the cluster along filaments of the large-scale structure.Conclusions. The observed galaxy content of A963 is a result of strongly anisotropic accretion of galaxies with different properties. Gas rich, star forming galaxies are being accreted from the east and west of the cluster and these galaxies are being quenched at r< R-200, likely by ram-pressure stripping. The bulk of the accretion onto the cluster, containing multiple groups, happens along the north-south axis and brings mostly passive galaxies, likely quenched before entering A963.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

    <a href="/en/project/GA19-18647S" target="_blank" >GA19-18647S: The origin of dark neutral gas structures around galaxies</a><br>

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2020

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Astronomy & Astrophysics

  • ISSN

    1432-0746

  • e-ISSN

  • Volume of the periodical

    638

  • Issue of the periodical within the volume

    June

  • Country of publishing house

    FR - FRANCE

  • Number of pages

    14

  • Pages from-to

    A126

  • UT code for WoS article

    000545015500001

  • EID of the result in the Scopus database

    2-s2.0-85088256716