output
19922026
most citedPlanck 2015 results. XIII. Cosmological parameters

10.6k citations

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astro-ph.CO2010

The intrinsic shape of bulges

J. Mendez-Abreu, E. Simonneau, J. A. L. Aguerri +1

The structural parameters of a magnitude-limited sample of 148 unbarred S0-Sb galaxies were derived using the GASP2D algorithm and then analyzed to derive the intrinsic shape of th…

astro-ph.GA2010★ 7 cited

A spectroscopic survey of faint, high-galactic latitude red clump stars. II. The medium resolution sample

T. Saguner, U. Munari, M. Fiorucci +1

Aims. The goal of our survey is to provide accurate and multi-epoch radial velocities, atmospheric parameters (Teff, log g and [M/H]), distances and space velocities of faint Red C…

astro-ph.CO2010★ 33 cited

An optical and HI study of the dwarf Local Group galaxy VV124=UGC4879. A gas-poor dwarf with a stellar disk?

M. Bellazzini, G. Beccari, T. A. Oosterloo +8

We present a detailed study of the dwarf galaxy VV124, recently recognized as a isolated member of the Local Group. We have obtained deep (r=26.5) wide-field g,r photometry of indi…

astro-ph.CO2010★ 4 cited

The jet of the BL Lacertae object PKS 2201+044: MAD near-IR adaptive optics observations and comparison with optical, radio and X-ray data

E. Liuzzo, R. Falomo, A. Treves +14

Relativistic jets are a common feature of radio loud active galactic nuclei. Multifrequency observations are a unique tool to constrain their physics. We report on a detailed study…

astro-ph.SR2010★ 94 cited

Fluorine and Sodium in C-rich low-metallicity stars

Sara Lucatello, Thomas Masseron, Jennifer A. Johnson +2

We present the N, O, F and Na abundance and 12C/13C isotopic ratio measurements or upper limits for a sample of 10 C-rich, metal-poor giant stars, eight enhanced in s-process (CEMP…

astro-ph.CO2010★ 35 cited

The evolution of early-type galaxies in clusters from z~ 0.8 to z~ 0: the ellipticity distribution and the morphological mix

Benedetta Vulcani, Bianca M. Poggianti, Alan Dressler +10

We present the ellipticity distribution and its evolution for early-type galaxies in clusters from z~0.8 to z~0, based on the WIde-field Nearby Galaxy-cluster Survey (WINGS)(0.04<z…