0484756 - ASÚ 2018 RIV GB eng J - Článek v odborném periodiku
Peters, T. - Naab, T. - Walch, S. - Glover, S.C.O. - Girichidis, P. - Pellegrini, E. - Klessen, R.S. - Wünsch, Richard - Gatto, A. - Baczynski, C.
The SILCC project IV. Impact of dissociating and ionizing radiation on the interstellar medium and Ha emission as a tracer of the star formation rate.
Monthly Notices of the Royal Astronomical Society. Roč. 466, č. 3 (2017), s. 3293-3308. ISSN 0035-8711. E-ISSN 1365-2966
Grant CEP: GA ČR GA15-06012S
Institucionální podpora: RVO:67985815
Klíčová slova: formation rate indicators * supernova-driven ism * molecular clouds
Obor OECD: Astronomy (including astrophysics,space science)
Impakt faktor: 5.194, rok: 2017 ; AIS: 1.41, rok: 2017
DOI: https://doi.org/10.1093/mnras/stw3216

We present three-dimensional radiation-hydrodynamical simulations of the impact of stellar winds, photoelectric heating, photodissociating and photoionizing radiation, and supernovae on the chemical composition and star formation in a stratified disc model. This is followed by a sink-based model for star clusters with populations of individual massive stars. Stellar winds and ionizing radiation regulate the star formation rate at a factor of similar to 10 below the simulation with only supernova feedback due to their immediate impact on the ambient interstellar medium after star formation. Ionizing radiation (with winds and supernovae) significantly reduces the ambient densities for most supernova explosions to. 10-25 g cm(-3), compared to 10-23g cm(-3) for the model with only winds and supernovae.
Trvalý link: http://hdl.handle.net/11104/0279901