output
19932026
most citedPlanck 2015 results. XIII. Cosmological parameters

10.6k citations

Showing 2006Show all

117 papers · 1 filter

astro-ph2006★ 28 cited

The He II Fowler lines and the O III and N III Bowen fluorescence lines in the symbiotic nova RR Tel

P. Selvelli, J. Danziger, P. Bonifacio

A new measure of reddening (E0.00) has been obtained from the comparison between the observed and the theoretical intensity decrement for 20 emission lines of the $…

astro-ph2006★ 23 cited

Beryllium abundance in turn-off stars of NGC 6752

Luca Pasquini, Piercarlo Bonifacio, Sofia Randich +3

Aims: To measure the beryllium abundance in two TO stars of the Globular Cluster NGC 6752, one oxygen rich and sodium poor, the other presumably oxygen poor and sodium rich. Be abu…

astro-ph2006★ 50 cited

Early Ultraviolet, Optical and X-Ray Observations of the Type IIP SN 2005cs in M51 with Swift

Peter J. Brown, Luc Dessart, Stephen T. Holland +14

We report early photospheric-phase observations of the Type IIP Supernova (SN) 2005cs obtained by Swift's Ultraviolet-Optical and X-Ray Telescopes. Observations started within two…

astro-ph2006★ 237 cited

The exotic chemical composition of the Sagittarius dwarf Spheroidal galaxy

L. Sbordone, P. Bonifacio, R. Buonanno +3

The Sagittarius dwarf Spheroidal galaxy is the nearest neighbor of the Milky Way. Moving along a short period quasi-polar orbit within the Halo, it is being destroyed by the tidal…

astro-ph2006★ 260 cited

REM observations of GRB 060418 and GRB 060607A: the onset of the afterglow and the initial fireball Lorentz factor determination

E. Molinari, S. D. Vergani, D. Malesani +32

Gamma-ray burst (GRB) emission is believed to originate in highly relativistic fireballs. Currently, only lower limits were securely set to the initial fireball Lorentz factor Gamm…

astro-ph2006★ 93 cited

MAGIC upper limits on the very high energy emission from GRBs

J. Albert, E. Aliu, H. Anderhub +57

The fast repositioning system of the MAGIC Telescope has allowed during its first data cycle, between 2005 and the beginning of year 2006, observing nine different GRBs as possible…