The white dwarf luminosity function
E García–Berro, TD Oswalt - New Astronomy Reviews, 2016 - Elsevier
White dwarfs are the final remnants of low-and intermediate-mass stars. Their evolution is
essentially a cooling process that lasts for∼ 10 Gyr. Their observed properties provide …
essentially a cooling process that lasts for∼ 10 Gyr. Their observed properties provide …
Cosmic chemical evolution with an early population of intermediate-mass stars
E Vangioni, J Silk, KA Olive… - Monthly Notices of the …, 2011 - academic.oup.com
We explore the effect of an early population of intermediate-mass stars in the 2–8 M⊙ range
on the cosmic chemical evolution. We discuss the implications of this population as it …
on the cosmic chemical evolution. We discuss the implications of this population as it …
The white dwarf population of tri‐axial haloes
S Torres, J Camacho, E García‐Berro - AIP Conference Proceedings, 2010 - pubs.aip.org
The nature of the several microlensing events observed by the MACHO team towards the
Large Magellanic Cloud (LMC) is still a controversial subject. Substellar objects and stars …
Large Magellanic Cloud (LMC) is still a controversial subject. Substellar objects and stars …