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20032014
most citedThe Hubble Ultra Deep Field

902 citations

Showing 2007Show all

12 papers · 1 filter

astro-ph200767 cited

A New Approach to the Study of Stellar Populations in Early-Type Galaxies: K-band Spectral Indices and an Application to the Fornax Cluster

D. R. Silva, H. Kuntschner, M. Lyubenova

New measurements of K-band spectral features are presented for eleven early-type galaxies in the nearby Fornax galaxy cluster. Based on these measurements, the following conclusion…

astro-ph2007

Spiral Galaxies in the SAURON Survey

Reynier F. Peletier, Katia Ganda, Jesus Falcon-Barroso +11

We discuss some recent integral field spectroscopy using the SAURON instrument of a sample consisting of 24 early-type spirals, part of the SAURON Survey, and 18 late-type spirals.…

astro-ph2007

Fast and Slow Rotators: The build-up of the Red Sequence

Eric Emsellem, Michele Cappellari, Davor Krajnovic +11

Using the unique dataset obtained within the course of the SAURON project, a radically new view of the structure, dynamics and stellar populations of early-type galaxies has emerge…

astro-ph20077 cited

Supermassive black holes from OASIS and SAURON integral-field kinematics

M. Cappellari, R. Bacon, R. L. Davies +10

Supermassive black holes are a key element in our understanding of how galaxies form. Most of the progress in this very active field of research is based on just ~30 determinations…

astro-ph20076 cited

UV and optical emission lines from the z=2.6 radio galaxy 0828+193: spatially resolved measurements

A. Humphrey, F. Iwamuro, M. Villar-Martin +3

We present an investigation into the spatial variation of the rest-frame UV and optical line and continuum emission along the radio axis of the z=2.6 radio galaxy 0828+193, using l…

astro-ph2007

HST's view of the youngest massive stars in the Magellanic Clouds

M. Heydari-Malayeri, M. R. Rosa, V. Charmandaris +5

Accurate physical parameters of newborn massive stars are essential ingredients to shed light on their formation, which is still an unsolved problem. The rare class of compact H II…