Zobrazeno 1 - 10
of 117
pro vyhledávání: '"Alejandro H Córsico"'
Autor:
Francisco C. De Gerónimo, Marcelo M. Miller Bertolami, Tiara Battich, Xiaodong Tang, Márcio Catelan, Alejandro H. Córsico, Yunjun Li, Xiao Fang, Leandro G. Althaus
Publikováno v:
The Astrophysical Journal, Vol 975, Iss 2, p 259 (2024)
Recent determinations of the total rate of the ^12 C+ ^12 C nuclear reaction show non-negligible differences with the reference reaction rate commonly used in previous stellar simulations. In addition, the current uncertainties in determining each ex
Externí odkaz:
https://doaj.org/article/e41051d3f1914a988f2cc219c79e2100
Publikováno v:
The Astrophysical Journal, Vol 964, Iss 1, p 30 (2024)
Breathing pulses are mixing episodes that could develop during the core helium-burning phase of low- and intermediate-mass stars. The occurrence of breathing pulses is expected to bear consequences on the formation and evolution of white dwarfs, part
Externí odkaz:
https://doaj.org/article/1ed884d885cf420db94a127c192e5b8a
Autor:
Alejandro H. Córsico
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 7 (2020)
In the course of their evolution, white-dwarf stars go through at least one phase of variability in which the global pulsations they undergo allow astronomers to peer into their interiors, making it possible to shed light on their deep inner structur
Externí odkaz:
https://doaj.org/article/a31f9e3ed81e4073a1d3601180744103
Autor:
Mukremin Kilic, Alejandro H Córsico, Adam G Moss, Gracyn Jewett, Francisco C De Gerónimo, Leandro G Althaus
We present APO and Gemini time-series photometry of WD J004917.14$-$252556.81, an ultramassive DA white dwarf with $T_{\rm eff} = 13020$ K and $\log{g} = 9.34$. We detect variability at two significant frequencies, making J0049$-$2525 the most massiv
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::99599363fa32d0cd3177da4f142e0d44
Autor:
Maria E Camisassa, Roberto Raddi, Leandro G Althaus, Jordi Isern, Alberto Rebassa-Mansergas, Santiago Torres, Alejandro H Córsico, Lydia Korre
Ultra-massive white dwarfs (1.05M⊙≲MWD) are particularly interesting objects that allow us to study extreme astrophysical phenomena such as type Ia supernovae explosions and merger events. Traditionally, ultra-massive white dwarfs are thoug
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9265905d199713512f38ab8858c23be8
https://hdl.handle.net/2117/386067
https://hdl.handle.net/2117/386067
Autor:
Murat Uzundag, Alejandro H Córsico, S O Kepler, Leandro G Althaus, Klaus Werner, Nicole Reindl, Maja Vučković
We present two new GW Vir-type pulsating white dwarf stars, TIC\,0403800675 (WD\,J115727.68-280349.64) and TIC\,1989122424 (WD J211738.38-552801.18) discovered in the Transiting Exoplanet Survey Satellite (TESS) photometric data. For both stars, the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::940638d0cf291c1843bfc09666312857
http://arxiv.org/abs/2204.02501
http://arxiv.org/abs/2204.02501
Autor:
María E Camisassa, Leandro G Althaus, Detlev Koester, Santiago Torres, Pilar Gil Pons, Alejandro H Córsico
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
Ultra-massive white dwarfs ($\rm M_{WD} \gtrsim 1.05\, M_{\odot}$) are considered powerful tools to study type Ia supernovae explosions, merger events, the occurrence of physical processes in the Super Asymptotic Giant Branch (SAGB) phase, and the ex
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7a6671c14783b955470706f0122b12c1
https://hdl.handle.net/2117/386112
https://hdl.handle.net/2117/386112
Autor:
Leandro G. Althaus, María E. Camisassa, Santiago Torres, Tiara Battich, Alejandro H. Córsico, Alberto Rebassa-Mansergas, Roberto Raddi
[Context] Ultra-massive white dwarfs (M ABSTRACT 1.05 M) are of utmost importance in view of the role they play in type Ia supernovae explosions, merger events, the existence of high-magnetic-field white dwarfs, and the physical processes in the supe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c6c79afa8bce59345551671e6185991c
http://hdl.handle.net/10261/295859
http://hdl.handle.net/10261/295859
Autor:
Gabriela Oliveira da Rosa, S. O. Kepler, Alejandro H. Córsico, J. E. S. Costa, J. J. Hermes, S. D. Kawaler, Keaton J. Bell, M. H. Montgomery, J. L. Provencal, D. E. Winget, G. Handler, Bart Dunlap, J. C. Clemens, Murat Uzundag
Publikováno v:
The Astrophysical Journal. 936:187
PG 1159-035 is the prototype of the DOV hot pre-white dwarf pulsators. It was observed during the Kepler satellite K2 mission for 69 days in 59 s cadence mode and by the TESS satellite for 25 days in 20 s cadence mode. We present a detailed asterosei
Autor:
Enrique Solano, Leandro Gabriel Althaus, F. M. Jiménez-Esteban, A Ferrer-Burjachs, Santiago Torres, Alberto Rebassa-Mansergas, Alejandro H. Córsico, Leila M. Calcaferro, Carlos Rodrigo
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Monthly Notices of the Royal Astronomical Society
Digital.CSIC. Repositorio Institucional del CSIC
instname
UPCommons. Portal del coneixement obert de la UPC
Universitat Politècnica de Catalunya (UPC)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Monthly Notices of the Royal Astronomical Society
Digital.CSIC. Repositorio Institucional del CSIC
instname
UPCommons. Portal del coneixement obert de la UPC
Universitat Politècnica de Catalunya (UPC)
We use the data provided by the Gaia Early Data Release 3 to search for a highly complete volume-limited sample of unresolved binaries consisting of a white dwarf and a main-sequence companion (i.e. WDMS binaries) within 100 pc. We select 112 objects
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ffb72236ca4c33b86acd0094d51f5d6f
https://academic.oup.com/mnras/advance-article/doi/10.1093/mnras/stab2039/6322850
https://academic.oup.com/mnras/advance-article/doi/10.1093/mnras/stab2039/6322850