Zobrazeno 1 - 6
of 6
pro vyhledávání: '"Stepien, Kazimierz"'
Autor:
Graczyk, Dariusz, Pietrzynski, Grzegorz, Thompson, Ian B., Gieren, Wolfgang, Pilecki, Bogumil, Konorski, Piotr, Villanova, Sandro, Gorski, Marek, Suchomska, Ksenia, Karczmarek, Paulina, Stepien, Kazimierz, Storm, Jesper, Taormina, Monica, Kolaczkowski, Zbigniew, Wielgorski, Piotr, Narloch, Weronika, Zgirski, Bartlomiej, Gallenne, Alexandre, Ostrowski, Jakub, Smolec, Radoslaw, Udalski, Andrzej, Soszynski, Igor, Kervella, Pierre, Nardetto, Nicolas, Szymanski, Michal K., Wyrzykowski, Lukasz, Ulaczyk, Krzysztof, Poleski, Radoslaw, Pietrukowicz, Pawel, Kozlowski, Szymon, Skowron, Jan, Mroz, Przemyslaw
Publikováno v:
ApJ, 2018, 860, 1
We present a determination of precise fundamental physical parameters of twenty detached, double- lined, eclipsing binary stars in the Large Magellanic Cloud (LMC) containing G- or early K-type giant stars. Eleven are new systems, the remaining nine
Externí odkaz:
http://arxiv.org/abs/1805.04952
Autor:
Pilecki, Bogumił, Gieren, Wolfgang, Smolec, Radosław, Pietrzyński, Grzegorz, Thompson, Ian B., Anderson, Richard I., Bono, Giuseppe, Soszyński, Igor, Kervella, Pierre, Nardetto, Nicolas, Taormina, Mónica, Stępień, Kazimierz, Wielgórski, Piotr
Publikováno v:
2017, Astrophysical Journal, 842, 110
We present the results of a study of the type II Cepheid ($P_{puls} = 4.974 d$) in the eclipsing binary system OGLE-LMC-T2CEP-098 ($P_{orb} = 397.2 d$). The Cepheid belongs to the peculiar W Vir group, for which the evolutionary status is virtually u
Externí odkaz:
http://arxiv.org/abs/1704.07782
Autor:
Stepien, Kazimierz, Kiraga, Marcin
Publikováno v:
A&A 577, A117 (2015)
It was recently demonstrated that contact binaries occur in globular clusters (GCs) only immediately below turn-off point and in the region of blue straggler stars (BSs). In addition, observations indicate that at least a significant fraction of BSs
Externí odkaz:
http://arxiv.org/abs/1503.07758
Autor:
Stepien, Kazimierz, Kiraga, Marcin
Publikováno v:
Acta Astronomica, v. 63, p 239 (2013)
[Abridged] We test the evolutionary model of cool close binaries on the observed properties of near contact binaries (NCBs). Those with a more massive component filling the Roche lobe are SD1 binaries whereas in SD2 binaries the Roche lobe filling co
Externí odkaz:
http://arxiv.org/abs/1403.2302
Akademický článek
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Autor:
STĘPIÉN, KAZIMIERZ
Publikováno v:
Publications of the Astronomical Society of the Pacific, 1968 Apr 01. 80(473), 220-222.
Externí odkaz:
https://www.jstor.org/stable/40674589