activity
19952009
most citedAges and metallicities of early-type galaxies in the SDSS: new insight into the physical origin of the colour-magnitude and the Mg2-sigmaV relations

386 citations · 4.7k across the 101 of their papers we have counts for

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Showing 2006Show all

29 papers · 1 filter

astro-ph20063 cited

Solar-like oscillation amplitudes and line-widths as a probe for turbulent convection in stars

R. Samadi, K. Belkacem, M. -J. Goupil +2

Excitation of solar-like oscillations is attributed to turbulent convection and takes place at the upper-most part of the outer convective zones. Amplitudes of these oscillations d…

astro-ph2006226 cited

First stars VII. Lithium in extremely metal poor dwarfs

P. Bonifacio, P. Molaro, T. Sivarani +12

Aims. This study aims to determine the level and constancy of the Spite plateau as definitively as possible from homogeneous high-quality VLT-UVES spectra of 19 of the most metal-p…

astro-ph200621 cited

Chandra point-source counts in distant galaxy clusters

M. Branchesi, I. M. Gioia, C. Fanti +2

With the superb angular resolution of the Chandra Observatory, it is now possible to detect X-ray point sources, either embedded in galaxy clusters or along the cluster line of sig…

astro-ph200642 cited

The stellar mass content of distant galaxy groups

Michael L. Balogh, Dave Wilman, Robert D. E. Henderson +8

We have obtained near-infrared imaging of 58 galaxy groups, in the redshift range 0.1<z<0.6, from the William Herschel Telescope and from the Spitzer IRAC data archive. The groups…

astro-ph20061 cited

Spectral analysis of X-ray pulsars with the INTEGRAL observatory

E. V. Filippova, S. S. Tsygankov, A. A. Lutovinov +1

We studied spectra for 34 accretion-powered X-ray and one millisecond pulsars that were within the field of view of the INTEGRAL observatory over two years (December 2002 - January…

astro-ph20061 cited

Pulse profiles and cyclotron line energy dependence on X-ray pulsars luminosity

S. Tsygankov, A. Lutovinov, E. Churazov +1

We present the results of broad band (3-100 keV) observations of several X-ray pulsars with the INTEGRAL and RXTE observatories. We concentrate on the luminosity and energy depende…