output
19932026
most citedPlanck 2015 results. XIII. Cosmological parameters

10.6k citations

Showing 2015 · astro-ph.SRShow all

15 papers · 2 filters

astro-ph.SR2015★ 42 cited

The spectacular evolution of Supernova 1996al over 15 years: a low energy explosion of a stripped massive star in a highly structured environment

Stefano Benetti, Nikolai N. Chugai, Victor P. Utrobin +9

Spectrophotometry of SN 1996al carried out throughout 15 years is presented. The early photometry suggests that SN 1996al is a Linear type-II supernova, with an absolute peak of Mv…

astro-ph.SR2015★ 38 cited

On the neutron-capture elements across the Galactic thin disk using Cepheids

R. da Silva, B. Lemasle, G. Bono +19

We present new accurate abundances for five neutron-capture (Y, La, Ce, Nd, Eu) elements in 73 classical Cepheids located across the Galactic thin disk. Individual abundances are b…

astro-ph.SR2015

The Carina Project IX: on Hydrogen and helium burning variables

G. Coppola, M. Marconi, P. B. Stetson +14

We present new multi-band (UBVI) time-series data of helium burning variables in the Carina dwarf spheroidal galaxy. The current sample includes 92 RR Lyrae-six of them are new ide…

astro-ph.SR2015★ 79 cited

Grid of theoretical NLTE equivalent widths of four Ba II lines and barium abundance in cool stars

S. A. Korotin, S. M. Andrievsky, C. J. Hansen +5

We present a grid of computed non-local thermodynamic equilibrium (NLTE) equivalent widths (EW) and NLTE abundance corrections for four Ba II lines: 4554, 5853, 6141, and 6496 A. T…

astro-ph.SR2015★ 89 cited

Early optical spectra of nova V1369 Cen show presence of Lithium

L. Izzo, M. Della Valle, E. Mason +10

We present early high resolution spectroscopic observations of the nova V1369 Cen. We have detected an absorption feature at 6695.6 Å\, that we have identified as blue--shifted $^7…

astro-ph.SR2015

Lithium evolution in metal-poor stars: from Pre-Main Sequence to the Spite plateau

Xiaoting Fu, Alessandro Bressan, Paolo Molaro +1

Lithium abundance derived in metal-poor main sequence stars is about three times lower than the value of primordial Li predicted by the standard Big Bang nucleosynthesis when the b…