most citedModeling He-rich subdwarfs through the hot-flasher Scenario

139 citations

9 papers

astro-ph200826 cited

WMAP 5-year constraints on time variation of and in a detailed recombination scenario

Claudia G. Scóccola, Susana. J. Landau, Hector Vucetich

We study the role of fundamental constants in an updated recombination scenario. We focus on the time variation of the fine structure constant, and the electron mass in the early U…

astro-ph2008139 cited

Modeling He-rich subdwarfs through the hot-flasher Scenario

M. M. Miller Bertolami, L. G. Althaus, K. Unglaub +1

We present 1D numerical simulations aimed at studying the hot-flasher scenario for the formation of He-rich subdwarf stars. Sequences were calculated for a wide range of metallicit…

astro-ph200858 cited

Galaxy populations in the Antlia cluster. I. Photometric properties of early-type galaxies

A. V. Smith Castelli, L. P. Bassino, T. Richtler +3

We present the first colour-magnitude relation (CMR) of early-type galaxies in the central region of the Antlia cluster, obtained from CCD wide-field photometry in the Washington p…

astro-ph200818 cited

Time variation of the electron mass in the early universe and the Barrow-Magueijo model

Claudia G. Scóccola, Mercedes E. Mosquera, Susana J. Landau +1

We put limits on the time variation of the electron mass in the early universe using observational primordial abundances of D, He4 and Li7, recent data from the Cosmic Microwave Ba…

astro-ph200753 cited

The pulsation modes of the pre-white dwarf PG 1159-035

J. E. S. Costa, S. O. Kepler, D. E. Winget +74

PG 1159-035, a pre-white dwarf with T_eff=140,000 K, is the prototype of both two classes: the PG1159 spectroscopic class and the DOV pulsating class. Previous studies of PG 1159-0…

astro-ph200787 cited

White Dwarf Luminosity and Mass Functions from Sloan Digital Sky Survey Spectra

Steven DeGennaro, Ted von Hippel, D. E. Winget +4

We present the first phase in our ongoing work to use Sloan Digital Sky Survey (SDSS) data to create separate white dwarf (WD) luminosity functions for two or more different mass r…