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Environmental Effects on ISM Content of Cluster galaxies

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F12%3A00389063" target="_blank" >RIV/67985815:_____/12:00389063 - isvavai.cz</a>

  • Result on the web

    <a href="http://dx.doi.org/10.1051/eas/1256015" target="_blank" >http://dx.doi.org/10.1051/eas/1256015</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1051/eas/1256015" target="_blank" >10.1051/eas/1256015</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Environmental Effects on ISM Content of Cluster galaxies

  • Original language description

    Galaxies in dense environments of clusters and groups are objects to ram pressure and hydrodynamical effects of the intra-cluster medium (ICM) that can significantly affect their interstellar content (ISM). We perform numerical simulations of the ram pressure stripping using tree/SPH code GADGET with an adapted method for calculating ISM-ICM interactions. We study the stripping effects of various environments of clusters, with compact or large distributions of the ICM, and the role of the disk tilt angle. Our results indicate that the total amount of the momentum transferred by the encountered ICM to the galaxy?s gas may provide the main features of the stripping. To reproduce our numerical results we propose a fitting formula relating the stripped mass fraction to the encountered ICM column density and the tilt angle. This dependence is superior to that on the peak ram pressure seen in Gunn and Gott criterion.

  • Czech name

  • Czech description

Classification

  • Type

    D - Article in proceedings

  • CEP classification

    BN - Astronomy and celestial mechanics, astrophysics

  • OECD FORD branch

Result continuities

  • Project

    <a href="/en/project/GP205%2F08%2FP556" target="_blank" >GP205/08/P556: Numerical simulations of environmental effects in galaxy clusters</a><br>

  • Continuities

    Z - Vyzkumny zamer (s odkazem do CEZ)

Others

  • Publication year

    2012

  • Confidentiality

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

Data specific for result type

  • Article name in the collection

    The Role of the Disk-Halo Interaction in Galaxy Evolution: Outflow vs. Infall?

  • ISBN

    9782759807871

  • ISSN

  • e-ISSN

  • Number of pages

    5

  • Pages from-to

    113-117

  • Publisher name

    EDP Sciences

  • Place of publication

    Cedex

  • Event location

    Espinho

  • Event date

    Aug 18, 2008

  • Type of event by nationality

    WRD - Celosvětová akce

  • UT code for WoS article

    000312968100013