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.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.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.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 |
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