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M. M. Miller Bertolami

Identifiers

  • name variant M. M. Miller Bertolami 0.60 · backfill

Papers (36)

  1. Stars on the ascending helium giant branch I. From white dwarf merger to helium giant: the evolutionary state of the rapidly rotating hot subdwarf HE 1518-0948 astro-ph.SR · 2026 · author #3
  2. Hot UV-bright stars of galactic globular clusters astro-ph.SR · 2019 · author #4
  3. Thermal torque effects on the migration of growing low-mass planets astro-ph.EP · 2019 · author #4
  4. The formation of giant planets in wide orbits by photoevaporation-synchronised migration astro-ph.EP · 2017 · author #2
  5. On the formation of DA white dwarfs with low hydrogen contents: Preliminary Results astro-ph.SR · 2016 · author #1
  6. Post-AGB evolution much faster than previously thought astro-ph.SR · 2016 · author #3
  7. Breaking news from the HST: The central star of the Stingray Nebula is now returning towards the AGB astro-ph.SR · 2016 · author #3
  8. Outer boundary conditions for evolving cool white dwarfs astro-ph.SR · 2012 · author #5
  9. Exploring the effects of detailed chemical profiles on the adiabatic oscillation spectrum of sdB stars: First Results astro-ph.SR · 2011 · author #1
  10. NSV 11749, an elder sibling of the born again stars V605 Aql and V4334 Sgr? astro-ph.SR · 2011 · author #1
  11. On the challenging variability of LS IV-14{\deg}116: pulsational instabilities excited by the {\epsilon}-mechanism astro-ph.SR · 2011 · author #1
  12. Constraining the axion mass through the asteroseismology of the ZZ Ceti star G117-B15A astro-ph.SR · 2011 · author #4
  13. The internal rotation of the GW Vir star PG 0112+200 through the eyes of asteroseismology astro-ph.SR · 2011 · author #4
  14. Probing the internal rotation of pre-white dwarf stars with asteroseismology: the case of PG 122+200 astro-ph.SR · 2011 · author #4
  15. Thermohaline mixing and the photospheric composition of low-mass giant stars astro-ph.SR · 2011 · author #2
  16. New chemical profiles for the asteroseismology of ZZ Ceti stars astro-ph.SR · 2010 · author #7
  17. New evolutionary sequences for hot H-deficient white dwarfs on the basis of a full account of progenitor evolution astro-ph.SR · 2009 · author #3
  18. On the possible existence of short-period g-mode instabilities powered by nuclear burning shells in post-AGB H-deficient (PG1159-type) stars astro-ph.SR · 2009 · author #3
  19. Evolution and colors of helium-core white dwarf stars with high-metallicity progenitors astro-ph.SR · 2009 · author #7
  20. Seismological constraints on the high-gravity DOV stars PG2131+066 and PG 1707+427 astro-ph.SR · 2009 · author #3
  21. Asteroseismology of hot pre-white dwarf stars: the case of the DOV stars PG 2131+066 and PG 1707+427, and the PNNV star NGC 1501 astro-ph.SR · 2009 · author #3
  22. On the formation of hot DQ white dwarfs astro-ph.SR · 2009 · author #4
  23. Modeling He-rich subdwarfs through the hot-flasher scenario (brief version) astro-ph · 2008 · author #1
  24. Revisiting the theoretical DBV (V777 Her) instability strip: the MLT theory of convection astro-ph · 2008 · author #3
  25. Modeling He-rich subdwarfs through the hot-flasher Scenario astro-ph · 2008 · author #1
  26. Evidence of thin helium envelopes in PG1159 stars astro-ph · 2008 · author #3
  27. Asteroseismological measurements on PG 1159-035, the prototype of the GW Vir variable stars astro-ph · 2007 · author #5
  28. On the systematics of asteroseismological mass determinations of PG1159 stars astro-ph · 2007 · author #4
  29. Asteroseismological constraints on the coolest GW Vir variable star (PG 1159-type)PG 0122+200 astro-ph · 2007 · author #2
  30. The born again (VLTP) scenario revisited: The mass of the remnants and implications for V4334 Sgr astro-ph · 2007 · author #1
  31. On the robustness of H-deficient post-AGB tracks astro-ph · 2007 · author #1
  32. Low-mass, helium-enriched PG1159 stars: a possible evolutionary origin and the implications for their pulsational stability properties astro-ph · 2007 · author #3
  33. Asteroseismological constraints on the pulsating planetary nebula nucleus (PG1159-type) RX J2117.1+3412 astro-ph · 2006 · author #3
  34. New nonadiabatic pulsation computations on full PG1159 evolutionary models: the theoretical GW Vir instability strip revisited astro-ph · 2006 · author #3
  35. New evolutionary calculations for the Born Again scenario astro-ph · 2005 · author #1
  36. The formation of DA white dwarfs with thin hydrogen envelopes astro-ph · 2005 · author #2

Mentions

  • 2604.11285 #3 · arxiv_oai · confidence 0.70 M. M. Miller Bertolami
  • 1209.2452 #5 · backfill · confidence 0.70 M. M. Miller Bertolami
  • 1111.2335 #1 · backfill · confidence 0.70 M. M. Miller Bertolami
  • 1111.2333 #1 · backfill · confidence 0.70 M. M. Miller Bertolami
  • 1109.4943 #1 · backfill · confidence 0.70 M. M. Miller Bertolami
  • 1108.3541 #4 · backfill · confidence 0.70 M. M. Miller Bertolami
  • 1108.3361 #4 · backfill · confidence 0.70 M. M. Miller Bertolami
  • 1108.3359 #4 · backfill · confidence 0.70 M. M. Miller Bertolami
  • 1104.0832 #2 · backfill · confidence 0.70 M. M. Miller Bertolami
  • 1005.2612 #7 · backfill · confidence 0.70 M. M. Miller Bertolami
  • 0909.2689 #3 · backfill · confidence 0.70 M. M. Miller Bertolami
  • 0906.2387 #3 · backfill · confidence 0.70 M. M. Miller Bertolami
  • 0905.1939 #7 · backfill · confidence 0.70 M. M. Miller Bertolami
  • 0903.3912 #3 · backfill · confidence 0.70 M. M. Miller Bertolami
  • 0903.3628 #3 · backfill · confidence 0.70 M. M. Miller Bertolami
  • 0901.1836 #4 · backfill · confidence 0.70 M. M. Miller Bertolami
  • 0810.4828 #1 · backfill · confidence 0.70 M. M. Miller Bertolami
  • 0810.2963 #3 · backfill · confidence 0.70 M. M. Miller Bertolami
  • 0808.3580 #1 · backfill · confidence 0.70 M. M. Miller Bertolami
  • 0802.3363 #3 · backfill · confidence 0.70 M. M. Miller Bertolami
  • 0712.0795 #5 · backfill · confidence 0.70 M. M. Miller Bertolami
  • 0710.3394 #4 · backfill · confidence 0.70 M. M. Miller Bertolami
  • 0709.0280 #2 · backfill · confidence 0.70 M. M. Miller Bertolami
  • 0706.0714 #1 · backfill · confidence 0.70 M. M. Miller Bertolami
  • 0706.0713 #1 · backfill · confidence 0.70 M. M. Miller Bertolami

Frequent Coauthors