Starburst triggered by compressive tides in galaxy mergers

Autor(en)
Florent Renaud, Christian Theis, Christian M. Boily
Abstrakt

The tidal field of galaxies is known generally to be disruptive. However, in the case of galaxy mergers, a compressive mode of tidal wave may develop and last long enough to cocoon the formation of star clusters. Using an N-body simulation of the Antennae galaxies, we derive the positions of these compressive regions and the statistics of their duration. Excellent agreement between the spatial distribution of tides and observed young clusters is found, while the characteristic e-folding times of 10 to 30 Myr derived for the tidal field compare well with cluster formation time-scales.

Organisation(en)
Institut für Astrophysik
Externe Organisation(en)
Université de Strasbourg
Journal
Astronomische Nachrichten
Band
329
Seiten
1050-1052
Anzahl der Seiten
3
ISSN
0004-6337
DOI
https://doi.org/10.1002/asna.200811083
Publikationsdatum
2008
ÖFOS 2012
103004 Astrophysik, 103003 Astronomie
Link zum Portal
https://ucrisportal.univie.ac.at/de/publications/82c49164-e612-4c1f-87a3-7d38a73a55bf