The origin of the [CII]-deficit in a simulated dwarf galaxies starburst

We present [CII] synthetic observations of smoothed particle hydrodynamics (SPH) simulations of a dwarf galaxy merger. The merging process varies the star-formation rate by more than three orders of magnitude. Several star clusters are formed, the feedback of which disperses and unbinds the dense ga...

Ausführliche Beschreibung

Bibliographische Detailangaben

Veröffentlicht in:	arXiv.org 2022-05
Hauptverfasser:	Bisbas, Thomas G, Walch, Stefanie, Naab, Thorsten, Lahén, Natalia, Herrera-Camus, Rodrigo, Steinwandel, Ulrich P, Fotopoulou, Constantina M, Chia-Yu, Hu, Johansson, Peter H
Format:	Artikel
Sprache:	eng
Schlagworte:	Dwarf galaxies Emission Explosions Far infrared radiation Galaxy mergers & collisions Luminosity Massive stars Physics - Astrophysics of Galaxies Simulation Smooth particle hydrodynamics Star clusters Star formation Stars & galaxies
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!