Zobrazeno 1 - 10
of 79
pro vyhledávání: '"M M Miller Bertolami"'
Autor:
B Montoro-Molina, M A Guerrero, B Pérez-Díaz, J A Toalá, S Cazzoli, M M Miller Bertolami, C Morisset
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
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The central star of the planetary nebula (PN) HuBi 1 has been recently proposed to have experienced a very late thermal pulse (VLTP), but the dilution of the emission of the recent ejecta by that of the surrounding H-rich old outer shell has so far h
Recently a new class of hot subluminous stars strongly enriched in C and O have been discovered (CO-sdOs). These stars show abundances very similar to those observed in PG1159 stars but at lower temperatures. Moreover, it has been recently suggested
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cbb69a314b95820e754168138c3cb152
http://arxiv.org/abs/2202.05635
http://arxiv.org/abs/2202.05635
Autor:
Paul G. Beck, M. G. Pedersen, Maria Bergemann, Vincent Van Eylen, Ignasi Ribas, Conny Aerts, Ian Czekala, Nicolas Lodieu, Eline Tolstoy, Marie Martig, Nate Bastian, Benard Nsamba, Davide Gandolfi, Ana Escorza, Keivan G. Stassun, Aldo Serenelli, George C. Angelou, Y. Lebreton, J. M. Bestenlehner, A. Moya, Krešimir Pavlovski, Achim Weiss, M. M. Miller Bertolami, J. S. G. Mombarg, D. Baroch, Victor Silva Aguirre, Diane Feuillet, Fabian Schneider, Juan Carlos Morales, Konstanze Zwintz, Mark Gieles, Nancy Elias-Rosa, Léo Girardi, Pier-Emmanuel Tremblay
Publikováno v:
The Astronomy and Astrophysics Review, 29, 1-141
The Astronomy and Astrophysics Review
Astronomy and Astrophysics Review
Astronomy and Astrophysics Review, Springer Verlag, 2021, 29 (1), pp.4. ⟨10.1007/s00159-021-00132-9⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Serenelli, A, Weiss, A, Aerts, C, Angelou, G C, Baroch, D, Bastian, N, Beck, P G, Bergemann, M, Bestenlehner, J M, Czekala, I, Elias-Rosa, N, Escorza, A, Van Eylen, V, Feuillet, D K, Gandolfi, D, Gieles, M, Girardi, L, Lebreton, Y, Lodieu, N, Martig, M, Miller Bertolami, M M, Mombarg, J S G, Morales, J C, Moya, A, Nsamba, B, Pavlovski, K, Pedersen, M G, Ribas, I, Schneider, F R N, Silva Aguirre, V, Stassun, K G, Tolstoy, E, Tremblay, P E & Zwintz, K 2021, ' Weighing stars from birth to death : mass determination methods across the HRD ', Astronomy and Astrophysics Review, vol. 29, no. 1, 4 . https://doi.org/10.1007/s00159-021-00132-9
Astronomy and Astrophysics Review, 2021, 29 (1), pp.4. ⟨10.1007/s00159-021-00132-9⟩
The Astronomy and Astrophysics Review, 29, 1, pp. 1-141
The Astronomy and Astrophysics Review
Astronomy and Astrophysics Review
Astronomy and Astrophysics Review, Springer Verlag, 2021, 29 (1), pp.4. ⟨10.1007/s00159-021-00132-9⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Serenelli, A, Weiss, A, Aerts, C, Angelou, G C, Baroch, D, Bastian, N, Beck, P G, Bergemann, M, Bestenlehner, J M, Czekala, I, Elias-Rosa, N, Escorza, A, Van Eylen, V, Feuillet, D K, Gandolfi, D, Gieles, M, Girardi, L, Lebreton, Y, Lodieu, N, Martig, M, Miller Bertolami, M M, Mombarg, J S G, Morales, J C, Moya, A, Nsamba, B, Pavlovski, K, Pedersen, M G, Ribas, I, Schneider, F R N, Silva Aguirre, V, Stassun, K G, Tolstoy, E, Tremblay, P E & Zwintz, K 2021, ' Weighing stars from birth to death : mass determination methods across the HRD ', Astronomy and Astrophysics Review, vol. 29, no. 1, 4 . https://doi.org/10.1007/s00159-021-00132-9
Astronomy and Astrophysics Review, 2021, 29 (1), pp.4. ⟨10.1007/s00159-021-00132-9⟩
The Astronomy and Astrophysics Review, 29, 1, pp. 1-141
The mass of a star is the most fundamental parameter for its structure, evolution, and final fate. It is particularly important for any kind of stellar archaeology and characterization of exoplanets. There exist a variety of methods in astronomy to e
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0989a27c3e883ec587ab4cf7d39bff9c
http://sedici.unlp.edu.ar/handle/10915/132501
http://sedici.unlp.edu.ar/handle/10915/132501
Autor:
Nicolás Cuello, Jorge Cuadra, Octavio Miguel Guilera, María Paula Ronco, M. M. Miller Bertolami, Pedro P. Poblete, Camilo Fontecilla, Amelia Bayo
The gas dissipation from a protoplanetary disk is one of the key processes affecting planet formation, and it is widely accepted that it happens on timescales of a few million years for disks around single stars. Over the last years, several protopla
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::52b0ede31b3bd67589024b564467552f
http://arxiv.org/abs/2105.09410
http://arxiv.org/abs/2105.09410
Autor:
María Paula Ronco, M. M. Miller Bertolami, Frédéric Masset, Julia Venturini, Octavio Miguel Guilera, J. Cuadra
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
A key process in planet formation is the exchange of angular momentum between a growing planet and the protoplanetary disc, which makes the planet migrate through the disc. Several works show that in general low-mass and intermediate-mass planets mig
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::99819b27a45777648677fff1bae2e6f9
Autor:
Martin A. Barstow, V. Schaffenroth, Sarah L. Casewell, Nicole Reindl, M. M. Miller Bertolami, S. Taubenberger, Nicolle L. Finch, Stephan Geier
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
The nucleus of the planetary nebula Hen2-428 is a short orbital-period (4.2h), double-lined spectroscopic binary, whose status as a potential supernova type Ia progenitor has raised some controversy in the literature. With the aim of resolving this d
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9b3f9ddcf4f5bfe08d12143d43f5d5ca
https://www.aanda.org/10.1051/0004-6361/202038117
https://www.aanda.org/10.1051/0004-6361/202038117
Autor:
Maurizio Salaris, V. Silva Aguirre, Santi Cassisi, Anwesh Mazumdar, Dennis Stello, George C. Angelou, Andrea Miglio, R. M. Ouazzani, Federico Spada, Earl P. Bellinger, Diego Bossini, Tiara Battich, M. M. Miller Bertolami, Jakob Rørsted Mosumgaard, Richard H. D. Townsend, K. B. Nielsen, Adriano Pietrinferni, Chen Jiang, S. Deheuvels, Saskia Hekker, A. Weiss, Jørgen Christensen-Dalsgaard, Aldo Serenelli, T. Constantino, Patrick Eggenberger, Yveline Lebreton
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2020, 635, pp.A165. ⟨10.1051/0004-6361/201935843⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Silva Aguirre, V, Christensen-Dalsgaard, J, Cassisi, S, Miller Bertolami, M, Serenelli, A, Stello, D, Weiss, A, Angelou, G, Jiang, C, Lebreton, Y, Spada, F, Bellinger, E P, Deheuvels, S, Ouazzani, R M, Pietrinferni, A, Mosumgaard, J R, Townsend, R H D, Battich, T, Bossini, D, Constantino, T, Eggenberger, P, Hekker, S, Mazumdar, A, Miglio, A, Nielsen, K B & Salaris, M 2020, ' The Aarhus red giants challenge. I. Stellar structures in the red giant branch phase ', Astronomy & Astrophysics, vol. 635, A164 . https://doi.org/10.1051/0004-6361/201935843
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 635, pp.A165. ⟨10.1051/0004-6361/201935843⟩
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Astronomy and Astrophysics-A&A, 2020, 635, pp.A165. ⟨10.1051/0004-6361/201935843⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Silva Aguirre, V, Christensen-Dalsgaard, J, Cassisi, S, Miller Bertolami, M, Serenelli, A, Stello, D, Weiss, A, Angelou, G, Jiang, C, Lebreton, Y, Spada, F, Bellinger, E P, Deheuvels, S, Ouazzani, R M, Pietrinferni, A, Mosumgaard, J R, Townsend, R H D, Battich, T, Bossini, D, Constantino, T, Eggenberger, P, Hekker, S, Mazumdar, A, Miglio, A, Nielsen, K B & Salaris, M 2020, ' The Aarhus red giants challenge. I. Stellar structures in the red giant branch phase ', Astronomy & Astrophysics, vol. 635, A164 . https://doi.org/10.1051/0004-6361/201935843
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 635, pp.A165. ⟨10.1051/0004-6361/201935843⟩
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
[Context] With the advent of space-based asteroseismology, determining accurate properties of red-giant stars using their observed oscillations has become the focus of many investigations due to their implications in a variety of fields in astrophysi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::32ca00bc11201ce0701dca512053533b
https://hal.science/hal-02523040/file/aa35843-19.pdf
https://hal.science/hal-02523040/file/aa35843-19.pdf
The treatment of convective boundaries remains an important source of uncertainty within stellar evolution, with drastic implications for the thermally-pulsing stars on the Asymptotic Giant Branch (AGB). Various sources are taken as motivation for th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::eee6cd745709c70497af9c6c10bc9153
http://arxiv.org/abs/2002.01860
http://arxiv.org/abs/2002.01860
Autor:
M. M. Miller Bertolami, Alejandro H. Córsico, Tiara Battich, Jørgen Christensen-Dalsgaard, Leandro Gabriel Althaus
Publikováno v:
Miller Bertolami, M M, Battich, T, Córsico, A H, Christensen-Dalsgaard, J & Althaus, L G 2020, ' Asteroseismic signatures of the helium core flash ', Nature Astronomy, vol. 4, no. 1, pp. 67-71 . https://doi.org/10.1038/s41550-019-0890-0
All evolved stars with masses $M_\star\lesssim 2M_\odot$ undergo a helium(He)-core flash at the end of their first stage as a giant star. Although theoretically predicted more than 50 years ago, this core-flash phase has yet to be observationally pro
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::be90e62b6e54d58f9f698a59cf6fa446
https://pure.au.dk/portal/da/publications/asteroseismic-signatures-of-the-helium-core-flash(2e08a368-3cee-466e-a43a-9c60fca99cda).html
https://pure.au.dk/portal/da/publications/asteroseismic-signatures-of-the-helium-core-flash(2e08a368-3cee-466e-a43a-9c60fca99cda).html
Autor:
M. M. Miller Bertolami, Robert A. Benjamin, Pierre Chayer, William V. Dixon, Andrea K. Dupree, S. V. Sosa Fiscella
Publikováno v:
The Astronomical Journal. 162:126
The Bright Star in the globular cluster 47 Tucanae (NGC 104) is a post-AGB star of spectral type B8 III. The ultraviolet spectra of late-B stars exhibit a myriad of absorption features, many due to species unobservable from the ground. The Bright Sta