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María E. Camisassa

3 papers here

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author2
  • last author1

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR2
  • astro-ph.GA1
ORCID 0000-0002-3524-190X

identity via Semantic Scholar / OpenAlex

activity
20152022
most citedThe white dwarf population of NGC 6397

33 citations · 57 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.SR2022★ 24 cited

Structure and evolution of ultra-massive white dwarfs in general relativity

L. G. Althaus, M. E. Camisassa, S. Torres +4

We present the first set of constant rest-mass ultra-massive oxygen/neon white dwarf cooling tracks with masses larger than 1.29 Msun which fully take into account the effects of g…

astro-ph.SR2020

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⋆​>1M⊙​) coming from single-star evolution are expected to harbor cores made of 16O and…

astro-ph.GA2015★ 33 cited

The white dwarf population of NGC 6397

S. Torres, E. García-Berro, L. G. Althaus +1

NGC 6397 is one of the most interesting, well observed and theoretically studied globular clusters. The existing wealth of observations allows us to study the reliability of the th…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.