Quenching and morphological transformation in semi-analytic models and CANDELS

R. Brennan, V. Pandya, R.~S. Somerville, G. Barro, E.~N. Taylor, S. Wuyts, E.~F. Bell, A. Dekel, H.~C. Ferguson, D.~H. McIntosh, C. Papovich, J. Primack

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Abstract

We examine the spheroid growth and star formation quenching experienced by galaxies since z ∼ 3 by studying the evolution with redshift of the quiescent and spheroid-dominated fractions of galaxies from the CANDELS (Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey) and GAMA (Galaxy and Mass Assembly) surveys. We compare the observed fractions with predictions from a semi-analytic model which includes prescriptions for bulge growth and AGN feedback due to mergers and disc instabilities. We facilitate direct morphological comparison by converting our model bulge-to-total stellar mass ratios to Sérsic indices. We then subdivide our population into the four quadrants of the specific star formation rate–Sérsic index plane and study the build-up of each of these subpopulations. We find that the fraction of star-forming discs declines steadily, while the fraction of quiescent spheroids builds up over cosmic time. The fractions of star-forming spheroids and quiescent discs are both non-negligible, and stay nearly constant over the period we have studied. Our model is qualitatively successful at reproducing the evolution of the two ‘main’ populations (star-forming discs and quiescent spheroids), and approximately reproduces the relative fractions of all four types, but predicts a stronger decline in star-forming spheroids, and increase in quiescent discs, than is seen in the observations. A model with an additional channel for bulge growth via disc instabilities agrees better overall with the observations than a model in which bulges can grow only through mergers. We also examine the relative importance of these different physical drivers of transformation (major and minor mergers and disc instabilities).
Original languageEnglish
Pages (from-to)2933-2956
Number of pages24
JournalMonthly Notices of the Royal Astronomical Society
Volume451
Issue number3
Early online date18 Jun 2015
DOIs
Publication statusPublished - 1 Aug 2015

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spheroids
near infrared
assembly
quenching
merger
stars
galaxies
subpopulation
quadrants
star formation rate
guy wires
stellar mass
mass ratios
star formation
prediction
predictions
index

Keywords

  • galaxies: bulges, galaxies: evolution, galaxies: interactions, galaxies: star formation

Cite this

Brennan, R., Pandya, V., Somerville, R. S., Barro, G., Taylor, E. N., Wuyts, S., ... Primack, J. (2015). Quenching and morphological transformation in semi-analytic models and CANDELS. Monthly Notices of the Royal Astronomical Society, 451(3), 2933-2956. https://doi.org/10.1093/mnras/stv1007

Quenching and morphological transformation in semi-analytic models and CANDELS. / Brennan, R.; Pandya, V.; Somerville, R.~S.; Barro, G.; Taylor, E.~N.; Wuyts, S.; Bell, E.~F.; Dekel, A.; Ferguson, H.~C.; McIntosh, D.~H.; Papovich, C.; Primack, J.

In: Monthly Notices of the Royal Astronomical Society, Vol. 451, No. 3, 01.08.2015, p. 2933-2956.

Research output: Contribution to journalArticle

Brennan, R, Pandya, V, Somerville, RS, Barro, G, Taylor, EN, Wuyts, S, Bell, EF, Dekel, A, Ferguson, HC, McIntosh, DH, Papovich, C & Primack, J 2015, 'Quenching and morphological transformation in semi-analytic models and CANDELS', Monthly Notices of the Royal Astronomical Society, vol. 451, no. 3, pp. 2933-2956. https://doi.org/10.1093/mnras/stv1007
Brennan, R. ; Pandya, V. ; Somerville, R.~S. ; Barro, G. ; Taylor, E.~N. ; Wuyts, S. ; Bell, E.~F. ; Dekel, A. ; Ferguson, H.~C. ; McIntosh, D.~H. ; Papovich, C. ; Primack, J. / Quenching and morphological transformation in semi-analytic models and CANDELS. In: Monthly Notices of the Royal Astronomical Society. 2015 ; Vol. 451, No. 3. pp. 2933-2956.
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