Zobrazeno 1 - 10
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pro vyhledávání: '"Berro E"'
The evolution of the remnant of the merger of two white dwarfs is still an open problem. Furthermore, few studies have addressed the case in which the remnant is a magnetic white dwarf with a mass larger than the Chandrasekhar limiting mass. Angular
Externí odkaz:
http://arxiv.org/abs/1804.01275
Recent Hubble Space Telescope observations have unveiled the white dwarf cooling sequence of the Galactic bulge. Although the degenerate sequence can be well fitted employing the most up-to-date theoretical cooling sequences, observations show a syst
Externí odkaz:
http://arxiv.org/abs/1802.00229
Autor:
Rebassa-Mansergas, A., Ren, J. J., Irawati, P., Garcia-Berro, E., Parsons, S. G., Schreiber, M. R., Gaensicke, B. T., Rodriguez-Gil, P., Liu, X., Manser, C., Palomo-Nevado, S., Jimenez-Ibarra, F., Costero, R., Echevarria, J., Michel, R., Zorotovic, M., Hollands, M., Han, Z., Luo, A., Villaver, E., Kong, X.
We present the second paper of a series of publications aiming at obtaining a better understanding regarding the nature of type Ia supernovae (SNIa) progenitors by studying a large sample of detached F, G and K main sequence stars in close orbits wit
Externí odkaz:
http://arxiv.org/abs/1708.09480
We present a Monte Carlo population synthesis study of white dwarf-main sequence (WD+MS) binaries in the Galactic disk aimed at reproducing the ensemble properties of the entire population observed by the Sloan Digital Sky Survey (SDSS) Data Release
Externí odkaz:
http://arxiv.org/abs/1705.05888
Autor:
Rebassa-Mansergas, A., Parsons, S. G., Garcia-Berro, E., Gaensicke, B. T., Schreiber, M. R., Rybicka, M., Koester, D.
The merger of close double white dwarfs (CDWDs) is one of the favourite evolutionary channels for producing Type Ia supernovae (SN Ia). Unfortunately, current theories of the evolution and formation of CDWDs are still poorly constrained and have seve
Externí odkaz:
http://arxiv.org/abs/1612.00217
Autor:
Rebassa-Mansergas, A., Anguiano, B., García-Berro, E., Freeman, K. C., Cojocaru, R., Manser, C. J., Pala, A. F., Gänsicke, B. T., Liu, X. -W.
The age-metallicity relation (AMR) is a fundamental observational constraint for understanding how the Galactic disc formed and evolved chemically in time. However, there is not yet an agreement on the observational properties of the AMR for the sola
Externí odkaz:
http://arxiv.org/abs/1608.03064
Publikováno v:
Classical and Quantum Gravity, 32, 165003, 2015
A feasible design for a magnetic diagnostics subsystem for eLISA will be based on that of its precursor mission, LISA Pathfinder. Previous experience indicates that magnetic field estimation at the positions of the test masses has certain complicatio
Externí odkaz:
http://arxiv.org/abs/1604.08563
Autor:
Rebassa-Mansergas, A., Ren, J. J., Parsons, S. G., Gaensicke, B. T., Schreiber, M. R., Garcia-Berro, E., Liu, X. -W., Koester, D.
We present an updated version of the spectroscopic catalogue of white dwarf-main sequence (WDMS) binaries from the Sloan Digital Sky Survey (SDSS). We identify 939 WDMS binaries within the data releases (DR) 9-12 of SDSS plus 40 objects from DR 1-8 t
Externí odkaz:
http://arxiv.org/abs/1603.01017
Autor:
Torres, S., García-Berro, E.
Publikováno v:
A&A 588, A35 (2016)
The white dwarf luminosity function is an important tool to understand the properties of the Solar neighborhood, like its star formation history, and its age. Here we present a population synthesis study of the white dwarf population within 40~pc fro
Externí odkaz:
http://arxiv.org/abs/1602.02533
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 theoretical white dwarf cooling sequences of low metallicity progenitors
Externí odkaz:
http://arxiv.org/abs/1507.08806