All

What are you looking for?

All
Projects
Results
Organizations

Quick search

  • Projects supported by TA ČR
  • Excellent projects
  • Projects with the highest public support
  • Current projects

Smart search

  • That is how I find a specific +word
  • That is how I leave the -word out of the results
  • “That is how I can find the whole phrase”

SILCC-Zoom: The early impact of ionizing radiation on forming molecular clouds

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F19%3A00521957" target="_blank" >RIV/67985815:_____/19:00521957 - isvavai.cz</a>

  • Result on the web

    <a href="https://doi.org/10.1093/mnras/sty2938" target="_blank" >https://doi.org/10.1093/mnras/sty2938</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1093/mnras/sty2938" target="_blank" >10.1093/mnras/sty2938</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    SILCC-Zoom: The early impact of ionizing radiation on forming molecular clouds

  • Original language description

    We present our first sub-parsec resolution radiation hydrodynamic simulations of two molecular clouds self-consistently forming from a turbulent, multiphase ISM. The clouds have similar initial masses of few 10(4) M-circle dot, escape velocities of -5 km s(-1), and a similar initial energy budget. We follow the formation of star clusters with a sink-based model and the impact of radiation from individual massive stars with the tree-based radiation transfer module TREERAY. Photoionizing radiation is coupled to a chemical network to follow gas heating, cooling, and molecule formation and dissociation. For the first 3 Myr of cloud evolution, we find that the overall star formation efficiency is considerably reduced by a factor of similar to 4 to global cloud values of < 10 per cent as the mass accretion of sinks that host massive stars is terminated after less than or similar to 1 Myr. Despite the low efficiency, star formation is triggered across the clouds.

  • 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/GB14-37086G" target="_blank" >GB14-37086G: Albert Einstein Center for Gravitation and Astrophysics</a><br>

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2019

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Monthly Notices of the Royal Astronomical Society

  • ISSN

    1365-2966

  • e-ISSN

  • Volume of the periodical

    482

  • Issue of the periodical within the volume

    3

  • Country of publishing house

    GB - UNITED KINGDOM

  • Number of pages

    22

  • Pages from-to

    4062-4083

  • UT code for WoS article

    000462312600084

  • EID of the result in the Scopus database

    2-s2.0-85067260292