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The CALIFA survey across the Hubble sequence Spatially resolved stellar population properties in galaxies?
(EDP Sciences, 2015)
Various di erent physical processes contribute to the star formation and stellar mass assembly histories of galaxies. One important approach to
understanding the significance of these di erent processes on galaxy evolution ...
The AIMSS Project, III : the stellar populations of compact stellar systems
(Wiley Blackwell Publishing, Inc, 2016-02)
In recent years, a growing zoo of compact stellar systems (CSSs) have been found whose physical properties (mass, size, velocity dispersion) place them between classical globular clusters (GCs) and true galaxies, leading ...
No direct coupling between bending of galaxy disc stellar age and light profiles
(Oxford University Press, 2016)
We study the stellar properties of 44 face-on spiral galaxies from the Calar Alto Legacy Integral Field Area survey via full spectrum fitting techniques. We compare the age profiles with the surface brightness distribution ...
Galaxy triplets in Sloan Digital Sky Survey Data Release 7: II. A connection with compact groups?
(Oxford University PressOxford, 2013)
We analyse a sample of 71 triplets of luminous galaxies derived from the work of O’Mill et al. We compare the properties of triplets and their members with those of control samples of compact groups, the 10 brightest members ...
A Megacam Survey of Outer Halo Satellites. VI. The Spatially resolved Starformation History of the Carina Dwarf Spheroidal Galaxy*
(IOP, 2016)
We present the spatially resolved star-formation history (SFH) of the Carina dwarf spheroidal galaxy, obtained from deep, wide-field g and r imaging and a metallicity distribution from the literature. Our photometry covers ...
SDSS-IV MaNGA: spatially resolved star formation histories in galaxies as a function of galaxy mass and type
(OXFORD UNIV PRESS, 2017)
We study the internal gradients of stellar population propertieswithin 1.5 R-e for a representative sample of 721 galaxies, with stellar masses ranging between 10(9)M circle dot and 10(11.5)M circle dot from the SDSS-IV ...