Galaxy and Mass Assembly (GAMA): time-scales for galaxies crossing the green valley. Issue 4 (16th March 2019)

• Record Type: Journal Article
• Authors: Phillipps, S; Bremer, M N; Hopkins, A M; De Propris, R; Taylor, E N; James, P A; Davies, L J M; Cluver, M E; Driver, S P; Eales, S A; Holwerda, B W; Kelvin, L S; Sansom, A E
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 485:Issue 4(2019)
• Page Start: 5559
• Page End: 5572
• Publication Date: 2019-03-16
• Subjects: galaxies: evolution -- galaxies: star formation -- galaxies: stellar content -- galaxies: structure; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/stz799
• Languages: English
• ISSNs: 0035-8711

Abstract

Abstract: We explore the constraints that can be placed on the evolutionary time-scales for typical low-redshift galaxies evolving from the blue cloud through the green valley and on to the red sequence. We utilize galaxies from the GAMA survey with 0.1 < z < 0.2 and classify them according to the intrinsic ( u * − r *) colours of their stellar populations, as determined by fits to their multiwavelength spectral energy distributions. Using these fits to also determine stellar population ages and star formation time-scales, we argue that our results are consistent with a green valley population dominated by galaxies that are simply decreasing their star formation (running out of gas) over a time-scale of 2–4 Gyr which are seen at a specific epoch in their evolution (approximately 1.6 e-folding times after their peak in star formation). If their fitted star formation histories are extrapolated forward, the green galaxies will further redden over time, until they attain the colours of a passive population. In this picture, no specific quenching event which cuts-off their star formation is required, though it remains possible that the decline in star formation in green galaxies may be expedited by internal or external forces. However, there is no evidence that green galaxies have recently changed their star formation time-scales relative to their previous longer term star formation histories.