Zobrazeno 1 - 5
of 5
pro vyhledávání: '"V. S. Radeva"'
Publikováno v:
AIP Conference Proceedings.
The paper aims to present the results achieved by students from the Naval Academy in Varna, who worked on a project of the educational program Simulation Exploration Experience (SEE) of the National Aeronautics and Space Administration (NASA) for the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a3029dd48e1af6e19e3d2d1a84bebaff
https://doi.org/10.1063/1.5082046
https://doi.org/10.1063/1.5082046
Autor:
J. G. Schmidt, N. Pawellek, Ł. Bukowiecki, M. M. Hohle, Markus Mugrauer, V. Krushevska, S. Meibom, Ronny Errmann, D. Tomono, Ľ. Hambálek, V. Yotov, B. Dincel, H. Takahashi, V. S. Radeva, Hiroshi Terada, Andrew W. Howard, Katharina Schreyer, Ch. Graefe, Grzegorz Nowak, Gracjan Maciejewski, Guillermo Torres, Ch. Adam, Martin Vaňko, Laurence A. Marschall, Yumiko Oasa, L. Trepl, Ch. Ginski, T. Eisenbeiß, X. Zhou, Dinko Dimitrov, T. O. B. Schmidt, C. Marka, Emil Kundra, S.C.-L. Hu, A. Dathe, J. Budaj, T. Pribulla, St. Raetz, Cesar Briceno, C. Broeg, Wen Ping Chen, Alfredo Sota, A. Berndt, M. Kitze, Aglae Kellerer, Zhenyu Wu, M. Fernandez, Ralph Neuhäuser, R. Chini, Diana P. Kjurkchieva, M. Moualla, M. Seeliger, S. Fiedler
Publikováno v:
Astronomische Nachrichten. 335:345-356
We report our investigation of the first transiting planet candidate from the YETI project in the young (~4 Myr old) open cluster Trumpler 37. The transit-like signal detected in the lightcurve of the F8V star 2M21385603+5711345 repeats every 1.36489
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::af646d0231398a46e5d5a3fff10be32f
https://doi.org/10.1002/asna.201412047
https://doi.org/10.1002/asna.201412047
Autor:
Tomáš Henych, Dinko Dimitrov, Ronny Errmann, Theodor Pribulla, M. Moualla, Ch. Adam, J. J. Downes, M. Seeliger, J. Gelszinnis, Jesús Hernández, Sven Buder, J. G. Schmidt, M. Kitze, L. Holmes, Ch. Ginski, T. Klocová, Xin Zhou, S. Czesla, V. S. Radeva, Hiromitsu Takahashi, Zhenyu Wu, Ralph Neuhäuser, Markus Mugrauer, M. Fernandez, M. M. Hohle, Alfredo Sota, N. Pawellek, T. O. B. Schmidt, C. Marka, S. Masda, St. Raetz, Cesar Briceno, Gracjan Maciejewski, L. Trepl, Diana P. Kjurkchieva
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
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Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 460(3), 2834-2852
instname
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 460(3), 2834-2852
Raetz, St. et. al.
CVSO 30 is a unique young low-mass system, because, for the first time, a close-in transiting and a wide directly imaged planet candidates are found around a common host star. The inner companion, CVSO 30 b, is the first possi
CVSO 30 is a unique young low-mass system, because, for the first time, a close-in transiting and a wide directly imaged planet candidates are found around a common host star. The inner companion, CVSO 30 b, is the first possi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fe5fcea8ccae50ca71167d5e037e8b33
Autor:
Diana P. Kjurkchieva, Evgeni Semkov, Sunay Ibryamov, K. A. Stoyanov, S. Peneva, I. K. Stateva, Dinko Dimitrov, T. R. Milanov, V. S. Radeva
Results from UBVRI photometric observations of the pre-main sequence star GM Cep obtained in the period April 2011 - August 2014 are reported in the paper. Presented data are a continuation of our photometric monitoring of the star started in 2008. G
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d8d45523a5bdd04ba15dcf3245760b0b
http://arxiv.org/abs/1502.07579
http://arxiv.org/abs/1502.07579
Autor:
U. Munari, E. de Miguel, R. D. Schwartz, Diana P. Kjurkchieva, Dinko Dimitrov, Stoyanka Peneva, Evgeni Semkov, V. S. Radeva, Milcho Tsvetkov, Rajka Jurdana-Šepić
Publikováno v:
Arias Montano. Repositorio Institucional de la Universidad de Huelva
instname
instname
We present new results from optical photometric and spectroscopic observations of the eruptive pre-main sequence star V2493 Cyg (HBC 722). The object has continued to undergo significant brightness variations over the past few months and is an ideal
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6ca6e2b5edc3f6ab03b85bff16913a2d
https://doi.org/10.1051/0004-6361/201219140
https://doi.org/10.1051/0004-6361/201219140