Zobrazeno 1 - 10
of 2 570
pro vyhledávání: '"Staels B."'
Autor:
Pieńkowski, D., Gałan, C., Tomov, T., Gazeas, K., Wychudzki, P., Mikołajewski, M., Kubicki, D., Staels, B., Zoła, S., Pakońska, P., Dȩbski, B., Kundera, T., Ogłoza, W., Dróżdż, M., Baran, A., Winiarski, M., Siwak, M., Dimitrov, D., Kjurkchieva, D., Marchev, D., Armiński, A., Miller, I., Kołaczkowski, Z., Moździerski, D., Zahajkiewicz, E., Bruś, P., Pigulski, A., Smela, T., Conseil, E., Boyd, D., Conidis, G. J., Plauchu-Frayn, I., Heras, T. A., Kardasis, E., Biskupski, M., Kneip, R., Hambálek, L., Pribulla, T., Kundra, E., Nedoroščik, J., Lopatovský, J., Garai, Z., Rodriguez, D., Kamiński, T., Dubois, F., Logie, L., Blanco, A. Capetillo, Kankiewicz, P., Świerczyński, E., Martignoni, M., Sergey, I., Qvam, J. Kare Trandem, Semkov, E., Ibryamov, S., Peneva, S., Carballo, J. -L. Gonzalez, Ribeiro, J., Dean, S., Apostolovska, G., Donchev, Z., Corp, L., McDonald, P., Rodriguez, M., Sanchez, A., Wiersema, K., Menke, J., Richardson, N.
Context. EE Cep is one of few eclipsing binary systems with a dark, dusty disk around an invisible object similar to {\epsilon} Aur. The system is characterized by grey and asymmetric eclipses every 5.6 yr, with a significant variation in their photo
Externí odkaz:
http://arxiv.org/abs/2001.05891
Publikováno v:
In Annales Pharmaceutiques Françaises March 2023 81(2):183-201
Publikováno v:
In La Presse Médicale Formation December 2022 3(6):499-506
Autor:
Aungwerojwit, A., Gänsicke, B. T., Wheatley, P. J., Pyrzas, S., Staels, B., Krajci, T., Rodríguez-Gil, P.
We present time-resolved photometry of a cataclysmic variable discovered in the Isaac Newton Telescope Photometric Halpha Survey of the northern galactic plane, IPHAS J062746.41+014811.3 and classify the system as the fourth deeply eclipsing intermed
Externí odkaz:
http://arxiv.org/abs/1209.0719
Autor:
Gałan, C., Mikołajewski, M., Tomov, T., Graczyk, D., Apostolovska, G., Barzova, I., Bellas-Velidis, I., Bilkina, B., Blake, R. M., Bolton, C. T., Bondar, A., Brát, L., Brożek, T., Budzisz, B., Cikała, M., Csák, B., Dapergolas, A., Dimitrov, D., Dobierski, P., Drahus, M., Dróżdż, M., Dvorak, S., Elder, L., Frcakowiak, S., Galazutdinov, G., Gazeas, K., Georgiev, L., Gere, B., Goździewski, K., Grinin, V. P., Gromadzki, M., Hajduk, M., Heras, T. A., Hopkins, J., Iliev, I., Janowski, J., Kocián, R., Kołaczkowski, Z., Kolev, D., Kopacki, G., Krzesiński, J., Kučáková, H., Kuligowska, E., Kundera, T., Kurpińska-Winiarska, M., Kuźmicz, A., Liakos, A., Lister, T. A., Maciejewski, G., Majcher, A., Majewska, A., Marrese, P. M., Michalska, G., Migaszewski, C., Miller, I., Munari, U., Musaev, F., Myers, G., Narwid, A., Németh, P., Niarchos, P., Niemczura, E., Ogłoza, W., Ögmen, Y., Oksanen, A., Osiwała, J., Peneva, S., Pigulski, A., Popov, V., Pych, W., Pye, J., Ragan, E., Roukema, B. F., Różański, P. T., Semkov, E., Siwak, M., Staels, B., Stateva, I., Stempels, H. C., Stȩślicki, M., Świerczyński, E., Szymański, T., Tomov, N., Waniak, W., Wieȩk, M., Winiarski, M., Wychudzki, P., Zajczyk, A., Zoła, S., Zwitter, T.
Two observational campaigns were carried out during the eclipses of EE Cep in 2003 and 2008/9 to verify whether the eclipsing body in the system is indeed a dark disk and to understand the observed changes in the depth and durations of the eclipses.
Externí odkaz:
http://arxiv.org/abs/1205.0028
Autor:
Pyrzas, S., Gaensicke, B. T., Thorstensen, J. R., Aungwerojwit, A, Boyd, D., Brady, S., Casares, J., Hickman, R. D. G., Marsh, T. R., Miller, I., Ogmen, Y., Pietz, J., Poyner, G., Rodriguez-Gil, P., Staels, B.
We identify HS 2325+8205 as an eclipsing, frequently outbursting dwarf nova with an orbital period of 279.841731(5) min. Spectroscopic observations are used to derive the radial velocity curve of the secondary star from absorption features and also f
Externí odkaz:
http://arxiv.org/abs/1201.6556
Autor:
Olech, A., de Miguel, E., Otulakowska, M., Thorstensen, J. R., Rutkowski, A., Novak, R., Masi, G., Richmond, M., Staels, B., Lowther, S., Stein, W., Ak, T., Boyd, D., Koff, R., Patterson, J., Eker, Z.
We report results of an extensive world-wide observing campaign devoted to the recently discovered dwarf nova SDSS J162520.29+120308.7 (SDSS J1625). The data were obtained during the July 2010 eruption of the star and in August and September 2010 whe
Externí odkaz:
http://arxiv.org/abs/1103.5754
We present the 2005-2010 outburst history of the SUUMa-type dwarf HS 0417+7445,along with a detailed analysis of extensive time-series photometry obtained in March 2008 during the second recorded superoutburst of the system. The mean outburst interva
Externí odkaz:
http://arxiv.org/abs/1011.1594
Autor:
Galan, C., Mikolajewski, M., Tomov, T., Swierczynski, E., Wiecek, M., Brozek, T., Maciejewski, G., Wychudzki, P., Hajduk, M., Rozanski, P. T., Ragan, E., Budzisz, B., Dobierski, P., Frackowiak, S., Kurpinska-Winiarska, M., Winiarski, M., Zola, S., Ogloza, W., Kuzmicz, A., Drozdz, M., Kuligowska, E., Krzesinski, J., Szymanski, T., Siwak, M., Kundera, T., Staels, B., Hopkins, J., Pye, J., Elder, L., Myers, G., Dimitrov, D., Popov, V., Semkov, E., Peneva, S., Kolev, D., Iliev, I., Barzova, I., Stateva, I., Tomov, N., Dvorak, S., Miller, I., Brat, L., Niarchos, P., Liakos, A., Gazeas, K., Pigulski, A., Kopacki, G., Narwid, A., Majewska, A., Steslicki, M., Niemczura, E., Ogmen, Y., Oksanen, A., Kucakova, H., Lister, T. A., Heras, T. A., Dapergolas, A., Bellas-Velidis, I., Kocian, R., Majcher, A.
The photometric and spectroscopic observational campaign organized for the 2008/9 eclipse of EE Cep revealed features, which indicate that the eclipsing disk in the EE Cep system has a multi-ring structure. We suggest that the gaps in the disk can be
Externí odkaz:
http://arxiv.org/abs/0910.0432
Autor:
Ness, J. -U., Drake, J. J., Beardmore, A. P., Boyd, D., Bode, M. F., Brady, S., Evans, P. A., Gaensicke, B. T., Kitamoto, S., Knigge, C., Miller, I., Osborne, J. P., Page, K. L., Rodriguez-Gil, P., Schwarz, G., Staels, B., Steeghs, D., Takei, D., Tsujimoto, M., Wesson, R., Zijlstra, A.
We describe the highly variable X-ray and UV emission of V458 Vul (Nova Vul 2007), observed by Swift between 1 and 422 days after outburst. Initially bright only in the UV, V458 Vul became a variable hard X-ray source due to optically thin thermal em
Externí odkaz:
http://arxiv.org/abs/0902.2199