output
19932026
most citedGaia Data Release 2. Summary of the contents and survey properties

8.6k citations

Showing 2000 · astro-phShow all

23 papers · 2 filters

astro-ph2000★ 526 cited

The O-Na and Mg-Al Anticorrelations in Turn-Off and early Subgiants in Globular Clusters

R. G. Gratton, P. Bonifacio, A. Bragaglia +16

High dispersion spectra (R>40,000) for a quite large number of stars at the main sequence turn-off and at the base of the subgiant branch in NGC6397 and NGC6752 were obtained with…

astro-ph2000★ 123 cited

Evidence for solar-like oscillations in beta Hydri

Timothy R. Bedding, R. Paul Butler, Hans Kjeldsen +6

We have made a clear detection of excess power, providing strong evidence for solar-like oscillations in the G2 subgiant beta Hyi. We observed this star over five nights with the U…

astro-ph2000★ 201 cited

Presupernova Evolution with Improved Rates for Weak Interactions

A. Heger, S. E. Woosley, G. Martinez-Pinedo +1

Recent shell-model calculations of weak-interaction rates for nuclei in the mass range A = 45 - 65 have resulted in substantial revisions to the hitherto standard set of Fuller, Fo…

astro-ph2000★ 10 cited

VLT identification of the optical afterglow of the gamma-ray burst GRB 000131 at z=4.50

M. I. Andersen, J. Hjorth, H. Pedersen +16

We report the discovery of the gamma-ray burst GRB 000131 and its optical afterglow. The optical identification was made with the VLT 84 hours after the burst following a BATSE det…

astro-ph2000

The Broken Light Curves of Gamma-Ray Bursts GRB 990123 and GRB 990510

S. Holland, G. Bjornsson, J. Hjorth +1

We have collected all of the published photometry for GRB 990123 and GRB 990510, the first two gamma-ray bursts where breaks were seen in the light curves of their optical afterglo…

astro-ph2000★ 5 cited

The beryllium abundance in the very metal-poor halo star G 64-12 from VLT/UVES observations

F. Primas, M. Asplund, P. E. Nissen +1

We report on a new spectroscopic analysis of the very metal deficient star G 64-12 ([Fe/H]=-3.3), aimed at determining, for the first time, its Be content. The spectra were observe…