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most citedEvolution of asymptotic giant branch stars I. Updated synthetic TP-AGB models and their basic calibration

411 citations · 1.8k across the 116 of their papers we have counts for

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25 papers · 1 filter

hep-ph2002

Frame Dependence of the Pair Contribution to the Pion Electromagnetic Form Factor in a Light-Front Approach

J. P. B. C. de Melo, T. Frederico, E. Pace +1

The frame dependence of the pair-term contribution to the electromagnetic form factor of the pion is studied within the Light Front approach. A symmetric ansatz for the pion Bethe-…

physics.atom-ph2002

133Cs87Rb Laser Cooled Dual Fountain

D. Calonico, Y. Sortais, S. Bize +5

At BNM-SYRTE laboratories in Paris two 133Cs fountains and a 87Rb one have been already demonstrated. This paper illustrates the construction of a 87Rb and Cs dual fountain realize…

astro-ph2002

AGNs among ROSAT Blank Field Sources

I. Cagnoni, M. Elvis, D. -W. Kim +3

We selected a sample of sources with high X-ray over optical flux ratio from the ROSAT PSPC archives. Out of the 16 sources in our sample, one is a (possibly extreme) BL Lac and tw…

astro-ph2002

Prospects for High Energy Studies of Pulsars with the AGILE Gamma-Ray Telescope

A. Pellizzoni, A. Chen, M. Conti +4

AGILE is a small gamma-ray astronomy satellite, with good spatial resolution, excellent timing capabilities and an unprecedented large field of view (~1/5 of the sky). It will be t…

astro-ph20022 cited

Mass-to-light ratios in early-type galaxies and the dark matter content

M. Capaccioli, N. R. Napolitano, M. Arnaboldi

The distribution of the radial trends of the mass-to-light ratios (M/L) within an assorted sample of early-type galaxies is discussed. Three classes of galaxies are identified acco…

astro-ph2002

The XMM-Newton view of the radio-quiet neutron star 1E 1207.4-5209

A. De Luca, S. Mereghetti, P. A. Caraveo +3

We have observed the radio-quiet X-ray pulsar 1E 1207.4-5209 with the high throughput EPIC cameras onboard XMM-Newton. The spectrum of this peculiar source is characterized by two…