activity
19992008
most citedWhite Dwarf Mass Distribution in the SDSS

329 citations · 776 across the 9 of their papers we have counts for

collaborators

9 papers

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-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-ph20071 cited

The importance of the remnant's mass for VLTP born again times. Implications for V4334 Sgr and V605 Aql

Marcelo M. Miller Bertolami, Leandro G. Althaus

We present numerical simulations of the very late thermal pulse (VLTP) scenario for a wide range of remnant masses. We show that, by taking into account the different possible remn…

astro-ph2007

Modeling He-rich subdwarfs through the Hot-Flasher scenario: First Results

Marcelo M. Miller Bertolami, Leandro G. Althaus

We present first results from evolutionary simulations aimed at exploring the Hot-Flasher scenario for the formation of H-deficient subdwarf stars. The two types of late hot flashe…

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…

astro-ph200740 cited

The born again (VLTP) scenario revisited: The mass of the remnants and implications for V4334 Sgr

M. M. Miller Bertolami, L. G. Althaus

We present 1-D numerical simulations of the very late thermal pulse (VLTP) scenario for a wide range of remnant masses. We show that by taking into account the different possible r…