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most citedStellar populations of early-type galaxies in different environments III. Line-strength gradients

83 citations · 155 across the 5 of their papers we have counts for

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astro-ph200814 cited

The Evolution Of Carbon, Sulphur, and Titanium Isotopes from High-Redshift to the Local Universe

G. L. Hughes, B. K. Gibson, L. Carigi +3

Recent observations of carbon, sulphur, and titanium isotopes at redshifts z~1 and in the local stellar disc and halo have opened a new window into the study of isotopic abundance…

astro-ph20063 cited

Chemodynamical Simulations of Elliptical Galaxies

Brad K. Gibson, Patricia Sanchez-Blazquez, Stephanie Courty +1

We review recent developments in the field of chemodynamical simulations of elliptical galaxies, highlighting (in an admittedly biased fashion) the work conducted with our cosmolog…

astro-ph200683 cited

Stellar populations of early-type galaxies in different environments III. Line-strength gradients

P. Sanchez-Blazquez, J. Gorgas, N. Cardiel

We present line-strength gradients for 22 spectral indices measured in a sample of 82 early-type galaxies in different environments,including the high-density core of the Coma clus…

astro-ph2005

An Imaging Study of the Globular Cluster Systems of NGC 1407 and NGC 1400

Duncan Forbes, Patricia Sanchez-Blazquez, Anna Phan +3

We present wide-field Keck telescope imaging of the globular cluster (GC) systems around NGC 1407 and NGC 1400 in the Eridanus galaxy cloud. This is complemented by Hubble Space Te…

astro-ph2004

On the Environmental Dependence of Cluster Galaxy Assembly Timescale

C. Carretero, A. Vazdekis, J. E. Beckman +2

We present estimates of CN and Mg overabundances with respect to Fe for early-type galaxies in 8 clusters over a range of richness and morphology. Spectra were taken from the Sloan…

astro-ph2004

Rings in the Haloes of Planetary Nebulae

R. L. M. Corradi, P. Sanchez-Blazquez, G. Mellema +2

We present a search for rings or arcs in the haloes of planetary nebulae (PNe). We discovered such structures in eight PNe, tripling the sample of PNe with known rings. This shows…