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The Origin of the Stellar Mass Distribution and Multiplicity
(Springer, 2020)
Evolution of low mass close binary systems with a neutron star: its dependence with the initial neutron star mass
(Wiley Blackwell Publishing, Inc, 2010-02)
We construct a set of binary evolutionary sequences for systems composed by a normal, solar composition, donor star together with a neutron star. We consider a variety of masses for each star as well as for the initial ...
New constraints for the initial-to-final mass relation of white dwarfs
(2020)
We present observational constraints for the initial-to-final mass relation (IFMR) derived from 11 white dwarfs (WDs) in wide binaries (WBs) that contain a turnoff/subgiant primary. Because the components of old-enough WBs ...
Mass loss and expansion of ultra compact dwarf galaxies through gas expulsion and stellar evolution for top-heavy stellar initial mass functions
(WILEY-BLACKWELL PUBLISHING, INC, 2010)
Thermogravimetry on calcined mass basis - hydrated cement phases and pozzolanic activity quantitative analysis
(Springer, 2009-07-01)
When cement hydrated compositions are analyzed by usual initial mass basis TG curves to calculate mass losses, the higher is the amount of additive added or is the combined water content, the higher is the cement 'dilution' ...
Thermogravimetry on calcined mass basis - hydrated cement phases and pozzolanic activity quantitative analysis
(Springer, 2009-07-01)
When cement hydrated compositions are analyzed by usual initial mass basis TG curves to calculate mass losses, the higher is the amount of additive added or is the combined water content, the higher is the cement 'dilution' ...