Zobrazeno 1 - 10
of 976
pro vyhledávání: '"Jerzykiewicz, M."'
Autor:
Jerzykiewicz, M., Pigulski, A., Michalska, G., Moździerski, D., Ratajczak, M., Handler, G., Moffat, A. F. J., Pablo, H., Popowicz, A., Wade, G. A., Zwintz, K.
Publikováno v:
Monthly Notices of the Royal Astronomical Society 503, 5554 (2021)
Results of an analysis of the BRITE-Constellation and SMEI photometry and radial-velocity observations, archival and new, of two single-lined spectroscopic binary systems $\nu$ Centauri and $\gamma$ Lupi are reported. In the case of $\gamma$ Lup AB,
Externí odkaz:
http://arxiv.org/abs/2104.11770
Autor:
Paszko T; Department of Chemistry, University of Life Sciences, Akademicka 15, 20-950, Lublin, Poland. tadeusz.paszko@up.lublin.pl., Spadotto CA; Embrapa Digital Agriculture, Av. André Tosello, 209, Campinas, SP, 13083-886, Brazil., Huber M; Department of Geology, Soil Science and Geoinformation, Maria Curie-Skłodowska University, Kraśnicka 2d/107, 20-718, Lublin, Poland., Jerzykiewicz M; Faculty of Chemistry, University of Wrocław, F. Joliot-Curie 4, 50-383, Wrocław, Poland., Matysiak J; Department of Chemistry, University of Life Sciences, Akademicka 15, 20-950, Lublin, Poland., Skrzypek A; Department of Chemistry, University of Life Sciences, Akademicka 15, 20-950, Lublin, Poland., Boguta P; Institute of Agrophysics, Polish Academy of Sciences, Doświadczalna 4, 20-290, Lublin, Poland.
Publikováno v:
Environmental science and pollution research international [Environ Sci Pollut Res Int] 2024 Nov 08. Date of Electronic Publication: 2024 Nov 08.
Autor:
Jerzykiewicz, M., Pigulski, A., Handler, G., Moffat, A. F. J., Popowicz, A., Wade, G. A., Zwintz, K., Pablo, H.
Results of an analysis of the BRITE-Constellation photometry of the SB1 system and ellipsoidal variable $\pi^5$ Ori (B2\,III) are presented. In addition to the orbital light-variation, which can be represented as a five-term Fourier cosine series wit
Externí odkaz:
http://arxiv.org/abs/2006.05178
Using BRITE photometric data for several close binary systems we address the problem of damping pulsations in close binary systems due to proximity effects. Because of small number statistics, no firm conclusion is given, but we find pulsations in th
Externí odkaz:
http://arxiv.org/abs/1711.10344
We present possible explanations of pulsations in early B-type main sequence stars which arise purely from the excitation of gravity modes. There are three stars with this type of oscillations detected from the BRITE light curves: $\kappa$ Cen, a Car
Externí odkaz:
http://arxiv.org/abs/1701.00961
Autor:
Weber J; Institute of Soil Science, Plant Nutrition and Environmental Protection, Wroclaw University of Environmental and Life Sciences, Grunwaldzka 53, 50-375 Wrocław, Poland., Jamroz E; Institute of Soil Science, Plant Nutrition and Environmental Protection, Wroclaw University of Environmental and Life Sciences, Grunwaldzka 53, 50-375 Wrocław, Poland., Mielnik L; Department of Bioengineering, West Pomeranian University of Technology in Szczecin, Papieża Pawła VI 3, 71-459 Szczecin, Poland., Spaccini R; Research Center CERMANU, University of Naples, Piazza Carlo di Borbone, 80055 Portici, Italy., Kocowicz A; Institute of Soil Science, Plant Nutrition and Environmental Protection, Wroclaw University of Environmental and Life Sciences, Grunwaldzka 53, 50-375 Wrocław, Poland., Ćwieląg-Piasecka I; Institute of Soil Science, Plant Nutrition and Environmental Protection, Wroclaw University of Environmental and Life Sciences, Grunwaldzka 53, 50-375 Wrocław, Poland., Jerzykiewicz M; Faculty of Chemistry, University of Wroclaw, 50-137 Wrocław, Poland., Parylak D; Institute of Agroecology and Plant Production, Wroclaw University of Environmental and Life Sciences, Grunwaldzki Sq. 24A, 50-363 Wrocław, Poland., Dębicka M; Institute of Soil Science, Plant Nutrition and Environmental Protection, Wroclaw University of Environmental and Life Sciences, Grunwaldzka 53, 50-375 Wrocław, Poland.
Publikováno v:
Molecules (Basel, Switzerland) [Molecules] 2024 Oct 25; Vol. 29 (21). Date of Electronic Publication: 2024 Oct 25.
Autor:
Jerzykiewicz, M., Handler, G., Daszynska-Daszkiewicz, J., Pigulski, A., Poretti, E., Rodriguez, E., Amado, P. J., Kolaczkowski, Z., Uytterhoeven, K., Dorokhova, T. N., Dorokhov, N. I., Lorenz, D., Zsuffa, D., Kim, S. -L., Bourge, P. -O., Acke, B., De Ridder, J., Verhoelst, T., Drummond, R., Movchan, A. I., Lee, J. -A., Steslicki, M., Molenda-Zakowicz, J., Garrido, R., Kim, S. -H., Michalska, G., Paparo, M., Antoci, V., Aerts, C.
A multisite photometric campaign for the Beta Cephei and eclipsing variable 16 Lacertae is reported. 749 h of high-quality differential photoelectric Stromgren, Johnson and Geneva time-series photometry were obtained with ten telescopes during 185 ni
Externí odkaz:
http://arxiv.org/abs/1508.05250
We present results of a search for identification of modes responsible for the six most significant frequency peaks detected in the rapidly rotating SPB star $\mu$ Eridani. All published and some unpublished photometric data are used in our new analy
Externí odkaz:
http://arxiv.org/abs/1410.6283
Autor:
Jerzykiewicz, M., Lehmann, H., Niemczura, E., Molenda-Żakowicz, J., Dymitrov, W., Fagas, M., Guenther, D. B., Hartmann, M., Hrudková, M., Kamiński, K., Moffat, A. F. J., Kuschnig, R., Leto, G., Matthews, J. M., Rowe, J. F., Ruciński, S. M., Sasselov, D., Weiss, W. W.
MOST time-series photometry of mu Eri, an SB1 eclipsing binary with a rapidly-rotating SPB primary, is reported and analyzed. The analysis yields a number of sinusoidal terms, mainly due to the intrinsic variation of the primary, and the eclipse ligh
Externí odkaz:
http://arxiv.org/abs/1303.6812
Autor:
Molenda-Zakowicz, J., Jerzykiewicz, M., Kopacki, G., Frasca, A., Catanzaro, G., Latham, D. W., Niemczura, E., Narwid, A., Steslicki, M., Arentoft, T., Kubat, J., Drobek, D., Dimitrow, W.
Publikováno v:
AIP Conference Proceedings 1170 (2009) 531-534
We summarize our ground-based program of spectroscopic and photometric observations of the asteroseismic targets of the Kepler space telescope. We have already determined atmospheric parameters, projected velocity of rotation, and radial velocity of
Externí odkaz:
http://arxiv.org/abs/1211.5247