Zobrazeno 1 - 10
of 50 978
pro vyhledávání: '"358"'
Publikováno v:
Finland Career Guide. 2006, p1. 7p.
Autor:
Washington, Jasmin E., Lewis, Hannah M., Anguiano, Borja, Majewski, Steven R., Chojnowski, S. Drew, Smith, Verne V., Stassun, Keivan G., Prieto, Carlos Allende, Cunha, Katia, Nidever, David L., Garcia-Hernandez, D. A., Pan, Kaike
LIN 358 and SMC N73 are two symbiotic binaries in the halo of the Small Magellanic Cloud, each composed of a hot white dwarf accreting from a cool giant companion. In this work, we characterize these systems using a combination of SED-fitting to the
Externí odkaz:
http://arxiv.org/abs/2107.08309
Autor:
Córsico, Alejandro H., Uzundag, Murat, Kepler, S. O., Silvotti, Roberto, Althaus, Leandro G., Koester, Detlev, Baran, Andrzej S., Bell, Keaton J., Bischoff-Kim, Agnès, Hermes, J. J., Kawaler, Steve D., Provencal, Judith L., Winget, Don E., Montgomery, Michael H., Bradley, Paul A., Kleinman, S. J., Nitta, Atsuko
Publikováno v:
A&A 659, A30 (2022)
The collection of high-quality photometric data by space telescopes is revolutionizing the area of white-dwarf asteroseismology. Among the different kinds of pulsating white dwarfs, there are those that have He-rich atmospheres, and they are called D
Externí odkaz:
http://arxiv.org/abs/2111.15551
Symbiotic binaries are long period interacting binaries consisting of a white dwarf (WD) accreting material from a cool evolved giant star via stellar winds. In this paper we study the symbiotic binary LIN 358 located in the SMC. We have observed LIN
Externí odkaz:
http://arxiv.org/abs/2011.02864
Autor:
Drapeau, Blanca
Publikováno v:
Agricultural History, 2021 Oct 01. 95(4), 705-707.
Externí odkaz:
https://www.jstor.org/stable/10.3098/ah.2021.095.4.705
Autor:
Bretzlaff-Holstein, Cini
Publikováno v:
Journal of Animal Ethics, 2021 Oct 01. 11(2), 112-113.
Externí odkaz:
https://www.jstor.org/stable/10.5406/janimalethics.11.2.0112
Autor:
Maccarini, Andrea M.
Publikováno v:
Slavonic and East European Review, 2021 Apr 01. 99(2), 390-392.
Akademický článek
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