Photoionising feedback in spiral arm molecular clouds

We present simulations of a 500 pc\(^2\) region, containing gas of mass 4 \(\times\) 10\(^6\) M\(_\odot\), extracted from an entire spiral galaxy simulation, scaled up in resolution, including photoionising feedback from stars of mass > 18 M\(_\odot\). Our region is evolved for 10 Myr and shows c...

Ausführliche Beschreibung

Bibliographische Detailangaben

Veröffentlicht in:	arXiv.org 2020-05
Hauptverfasser:	Bending, Thomas J R, Dobbs, Clare L, Bate, Matthew R
Format:	Artikel
Sprache:	eng
Schlagworte:	Clumps Compressed gas Feedback Galaxies Molecular clouds Particle mass Photoionization Physics - Astrophysics of Galaxies Simulation Spiral galaxies Star & galaxy formation Star clusters Star formation rate Stellar evolution
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!