Zobrazeno 1 - 6
of 6
pro vyhledávání: '"DrahomÍr Chochol"'
Autor:
Sergei Yu. Shugarov, Vitalij P. Goranskij, Nataly A. Katysheva, Anatolij V. Kusakin, Nataly V. Metlova, Igor M. Volkov, DrahomÍr Chochol, Theodor Pribulla, Eugenia A. Karitskaja, Alon Retter, Ohad Shemmer, Yiftah Lipkin
Publikováno v:
Astrophysics and Space Science. 296:431-434
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8a349229cf2b612646c971b1dbbc8fd2
https://doi.org/10.1007/s10509-005-4864-6
https://doi.org/10.1007/s10509-005-4864-6
Publikováno v:
Astrophysics and Space Science. 296:281-284
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::333c6baba280da78b27a6428596ad569
https://doi.org/10.1007/s10509-005-4831-2
https://doi.org/10.1007/s10509-005-4831-2
Autor:
Helen Rovithis-Livaniou, Sotirios Tsantilas, Peter Rovithis, DrahomÍr Chochol, AugustÍn Skopal, Theodor Pribulla
Publikováno v:
Astrophysics and Space Science. 296:101-104
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::706d4e5f8f7eb0aeecfa5dba1866367e
https://doi.org/10.1007/s10509-005-4388-0
https://doi.org/10.1007/s10509-005-4388-0
Autor:
Theodor Pribulla, Martin Vaňko, Drahomír Chochol, L’ubomıır Hambálek, Štefan Parimucha, Vicky Kologera, Marc van der Sluys
Publikováno v:
AIP Conference Proceedings.
O’Connell effect in early‐type close eclipsing binaries is not caused by solar‐type spots. In most early‐type contact binaries it has the same sign: maximum following the primary minimum being the brighter of the two. Broadening functions of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::50707f6496a3a581ea97eb6175923c33
https://doi.org/10.1063/1.3536405
https://doi.org/10.1063/1.3536405
Autor:
Drahomír Chochol, Natalia A. Katysheva, Sergey Yu. Shugarov, Igor M. Volkov, Maxim V. Andreev, Vicky Kologera, Marc van der Sluys
Publikováno v:
AIP Conference Proceedings.
Time series analysis of multicolour CCD photometry of a new WZ Sge‐type dwarf nova V466 And, discovered during its superoutburst in September 2008, revealed the early superhumps, with the period 0.056383 d in the first 11 days, the ordinary superhu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d32b5dc9c8d470c5c236e87ef34f1e0f
https://doi.org/10.1063/1.3536369
https://doi.org/10.1063/1.3536369
Publikováno v:
Close Binaries in the 21st Century: New Opportunities and Challenges ISBN: 9781402050268
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::22ae4206ca42836b809f4117122e1f5e
https://doi.org/10.1007/978-1-4020-5027-5_9
https://doi.org/10.1007/978-1-4020-5027-5_9
