Mergers, starbursts, and quenching in the SIMBA simulation

dc.contributor.author	davé, romeel
dc.date.accessioned	2022-12-05T10:53:00Z
dc.date.available	2022-12-05T10:53:00Z
dc.date.issued	2019
dc.identifier.citation	Francisco Rodríguez Montero, Romeel Davé, Vivienne Wild, Daniel Anglés-Alcázar, Desika Narayanan, Mergers, starbursts, and quenching in the SIMBA simulation, Monthly Notices of the Royal Astronomical Society, Volume 490, Issue 2, December 2019, Pages 2139–2154, https://doi.org/10.1093/mnras/stz2580	en_US
dc.identifier.issn	2331-8422
dc.identifier.uri	http://hdl.handle.net/10566/8225
dc.description.abstract	We use the SIMBAcosmological galaxy formation simulation to investigate the relationship between major mergers (4:1), starbursts, and galaxy quenching. Mergers are identified via sudden jumps in stellar mass M∗ well above that expected from in situ star formation, while quenching is defined as going from specific star formation rate (sSFR) > t−1 H to < 0.2t −1 H , where tH is the Hubble time.	en_US
dc.language.iso	en_US	en_US
dc.publisher	Oxford Academic	en_US
dc.subject	galaxies	en_US
dc.subject	evolution	en_US
dc.subject	formation	en_US
dc.title	Mergers, starbursts, and quenching in the SIMBA simulation	en_US
dc.type	Article	en_US