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M. M. Miller Bertolami

3 papers hereh-index 12458 citations39 works total

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

author position
  • middle author3

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

fields
  • astro-ph.SR2
  • astro-ph1
same name
  • M. M. Miller Bertolami — 2 papers

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

most citedEvidence of thin helium envelopes in PG1159 stars

27 citations · 73 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.SR2009★ 21 cited

On the possible existence of short-period g-mode instabilities powered by nuclear burning shells in post-AGB H-deficient (PG1159-type) stars

A. H. Córsico, L. G. Althaus, M. M. Miller Bertolami +2

We present a pulsational stability analysis of hot post-AGB H-deficient pre-white dwarf stars with active He-burning shells. The stellar models employed are state-of-the-art equili…

astro-ph.SR2009★ 25 cited

On the formation of hot DQ white dwarfs

L. G. Althaus, E. García-Berro, A. H. Córsico +2

We present the first full evolutionary calculations aimed at exploring the origin of hot DQ white dwarfs. These calculations consistently cover the whole evolution from the born-ag…

astro-ph2008★ 27 cited

Evidence of thin helium envelopes in PG1159 stars

L. G. Althaus, A. H. Córsico, M. M. Miller Bertolami +2

We present evidence that PG1159 stars could harbour He--rich envelopes substantially thinner than those predicted by current evolutionary models with current estimates of mass loss…

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