New fully evolutionary models for asteroseismology of ultra-massive white dwarf stars

A. H. Córsico, F. C. De Gerónimo, M. E. Camisassa +1

Ultra-massive hydrogen-rich (DA spectral type) white dwarf (WD) stars ($M_{\star }>1M_{\odot }$) coming from single-star evolution are expected to harbor cores made of ${}^{16}$O and…