Simulations of ram-pressure stripping in galaxy-cluster interactions

Context. Observationally, the quenching of star-forming galaxies appears to depend both on their mass and environment. The exact cause of the environmental dependence is still poorly understood, yet semi-analytic models (SAMs) of galaxy formation need to parameterise it to reproduce observations of...

Ausführliche Beschreibung

Bibliographische Detailangaben

Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2016-07, Vol.591, p.A51
Hauptverfasser:	Steinhauser, Dominik, Schindler, Sabine, Springel, Volker
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomical models Computer simulation Disk galaxies Disks Galaxies galaxies: clusters: general galaxies: evolution galaxies: interactions galaxies: star formation methods: numerical Quenching Star formation Stripping
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!