Journal: Monthly Notices of the Royal Astronomical Society
Publication
Stellar migration in the Auriga simulations
We study the presence and importance of stellar migration in the evolution of 17 Milky-Way like disc galaxies with stellar mass 10 < log(M */M ⊙) < 11 from the...
Stellar population synthesis models between 2.5 and 5 μm based on the empirical IRTF stellar library
We present the first single-burst stellar population models in the infrared wavelength range between 2.5 and 5 μm which are exclusively based on empirical...
Stellar populations and physical properties of starbursts in the antennae galaxy from self-consistent modelling of MUSE spectra
We have modelled the stellar and nebular continua and emission-line intensity ratios of massive stellar populations in the Antennae galaxy using high resolution...
Stellar populations and surface brightness fluctuations: new observations and models
We investigate the use of surface brightness fluctuations (SBF) measurements in optical and near-IR bandpasses for both stellar population and distance studies...
Stellar populations in the centres of brightest cluster galaxies
This paper is part of a series devoted to the study of the stellar populations in brightest cluster galaxies (BCGs), aimed at setting constraints on the...
Stellar populations of bulges in 14 cluster disc galaxies
Photometry and long-slit spectroscopy are presented for 14 S0 and spiral galaxies of the Fornax, Eridanus and Pegasus cluster, and NGC 7582 group. The...
Stellar populations of massive elliptical galaxies in very rich clusters
We present a detailed stellar population analysis of 27 massive elliptical galaxies within four very rich clusters at redshift z ~ 0.2: A115, A655, A963 and...
Stellar spectral models compared with empirical data
The empirical MILES stellar library is used to test the accuracy of three different, state-of-the-art, theoretical model libraries of stellar spectra. These...
Stellar splashback: the edge of the intracluster light
We examine the outskirts of galaxy clusters in the C-EAGLE simulations to quantify the 'edges' of the stellar and dark matter distribution. The radius of the...