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Why do many early-type galaxies lack emission lines? I. Fossil clues
F Herpich, G Stasińska, A Mateus, N Vale Asari and R Cid Fernandes Monthly Notices of the Royal Astronomical Society 481(2) 1774 (2018) https://doi.org/10.1093/mnras/sty2391
Cosmic Star Formation: A Simple Model of the SFRD(z)
Cesare Chiosi, Mauro Sciarratta, Mauro D’Onofrio, Emanuela Chiosi, Francesca Brotto, Rosaria De Michele and Valeria Politino The Astrophysical Journal 851(1) 44 (2017) https://doi.org/10.3847/1538-4357/aa99d5
Effect of the star formation histories on theSFR-M∗relation atz≥ 2
Evolution of thermally pulsing asymptotic giant branch stars – III. Dust production at supersolar metallicities★
Ambra Nanni, Alessandro Bressan, Paola Marigo and Léo Girardi Monthly Notices of the Royal Astronomical Society 438(3) 2328 (2014) https://doi.org/10.1093/mnras/stt2348
Modelling element abundances in semi-analytic models of galaxy formation
Robert M. Yates, Bruno Henriques, Peter A. Thomas, et al. Monthly Notices of the Royal Astronomical Society 435(4) 3500 (2013) https://doi.org/10.1093/mnras/stt1542
The two regimes of the cosmic sSFR evolution are due to spheroids and discs
Evolution of thermally pulsing asymptotic giant branch stars – II. Dust production at varying metallicity
Ambra Nanni, Alessandro Bressan, Paola Marigo and Léo Girardi Monthly Notices of the Royal Astronomical Society 434(3) 2390 (2013) https://doi.org/10.1093/mnras/stt1175
INVESTIGATING THE POTENTIAL DILUTION OF THE METAL CONTENT OF HOT GAS IN EARLY-TYPE GALAXIES BY ACCRETED COLD GAS