Zobrazeno 1 - 10
of 166
pro vyhledávání: '"Stachowski G"'
Autor:
Marciniak, A., Ďurech, J., Alí-Lagoa, V., Ogłoza, W., Szakáts, R., Müller, T. G., Molnár, L., Pál, A., Monteiro, F., Arcoverde, P., Behrend, R., Benkhaldoun, Z., Bernasconi, L., Bosch, J., Brincat, S., Brunetto, L., Bąk, M. Butkiewicz, Del Freo, F., Duffard, R., Evangelista-Santana, M., Farroni, G., Fauvaud, S., Fauvaud, M., Ferrais, M., Geier, S., Golonka, J., Grice, J., Hirsch, R., Horbowicz, J., Jehin, E., Julien, P., Kalup, Cs., Kamiński, K., Kamińska, M. K., Kankiewicz, P., Kecskeméthy, V., Kim, D. -H., Kim, M. -J., Konstanciak, I., Krajewski, J., Kudak, V., Kulczak, P., Kundera, T., Lazzaro, D., Manzini, F., Medeiros, H., Michimani-Garcia, J., Morales, N., Nadolny, J., Oszkiewicz, D., Pakštienė, E., Pawłowski, M., Perig, V., Pilcher, F., Pinel, P., Podlewska-Gaca, E., Polakis, T., Richard, F., Rodrigues, T., Rondon, E., Roy, R., Sanabria, J. J., Santana-Ros, T., Skiff, B., Skrzypek, J., Sobkowiak, K., Sonbas, E., Stachowski, G., Strajnic, J., Trela, P., Tychoniec, Ł., Urakawa, S., Verebelyi, E., Wagrez, K., Żejmo, M., Żukowski, K.
Publikováno v:
A&A 654, A87 (2021)
Results from the TESS mission showed that previous studies strngly underestimated the number of slow rotators, revealing the importance of studying those asteroids. For most slowly rotating asteroids (P > 12), no spin and shape model is available bec
Externí odkaz:
http://arxiv.org/abs/2109.00463
Autor:
Gazeas, K., Zola, S., Liakos, A., Zakrzewski, B., Rucinski, S. M., Kreiner, J. M., Ogloza, W., Drozdz, M., Koziel-Wierzbowska, D., Stachowski, G., Siwak, M., Baran, A., Kjurkchieva, D., Marchev, D., Erdem, A., Szalankiewicz, S.
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 2021, Volume 501, Issue 2, pp.2897-2919
This paper presents the results of a combined spectroscopic and photometric study of 20 contact binary systems: HV Aqr, OO Aql, FI Boo, TX Cnc, OT Cnc, EE Cet, RWCom, KR Com, V401 Cyg, V345 Gem, AK Her, V502 Oph, V566 Oph, V2612 Oph, V1363 Ori, V351
Externí odkaz:
http://arxiv.org/abs/2101.10680
Publikováno v:
A&A 642, A105 (2020)
In this study, we independently test the presence of an exoplanet around the binary KIC 9472174, which is composed of a red dwarf and a pulsating type B subdwarf. We also present the results of our search for Jupiter-mass objects orbiting near to the
Externí odkaz:
http://arxiv.org/abs/2009.02749
Autor:
Bhatta, G., Stawarz, L., Markowitz, A., Balasubramaniam, K., Zola, S., Zdziarski, A. A., Jamrozy, M., Ostrowski, M., Kuzmicz, A., Ogloza, W., Drozdz, M., Siwak, M., Koziel-Wierzbowska, D., Debski, B., Kundera, T., Stachowski, G., Machalski, J., Paliya, V. S., Caton, D. B.
Here we explore the disk-jet connection in the broad-line radio quasar 4C+74.26, utilizing the results of the multiwavelength monitoring of the source. The target is unique in that its radiative output at radio wavelengths is dominated by a moderatel
Externí odkaz:
http://arxiv.org/abs/1805.06957
Autor:
Suchanicz, J., Kluczewska-Chmielarz, K., Nowakowska-Malczyk, M., Jagło, G., Stachowski, G., Kruzina, T.V.
Publikováno v:
In Journal of Alloys and Compounds 5 August 2022 911
Autor:
Marciniak, A., Pilcher, F., Oszkiewicz, D., Santana-Ros, T., Urakawa, S., Fauvaud, S., Kankiewicz, P., Tychoniec, Ł., Fauvaud, M., Hirsch, R., Horbowicz, J., Kamiński, K., Konstanciak, I., Kosturkiewicz, E., Murawiecka, M., Nadolny, J., Nishiyama, K., Okumura, S., Polińska, M., Richard, F., Sakamoto, T., Sobkowiak, K., Stachowski, G., Trela, P.
Publikováno v:
Marciniak et al. 2015, PSS, 118, 256
Physical studies of asteroids depend on an availability of lightcurve data. Targets that are easy to observe and analyse naturally have more data available, so their synodic periods are confirmed from multiple sources. Also, thanks to availability of
Externí odkaz:
http://arxiv.org/abs/1711.02429
Autor:
Bhatta, G., Zola, S., Stawarz, Ł., Ostrowski, M., Winiarski, M., Ogłoza, W., Dróżdz, M., Siwak, M., Liakos, A., Kozieł-Wierzbowska, D., Gazeas, K., Debski, B., Kundera, T., Stachowski, G., Paliya, V. S.
Detection of periodicity in the broad-band non-thermal emission of blazars has so far been proven to be elusive. However, there are a number of scenarios which could lead to quasi-periodic variations in blazar light curves. For example, orbital or th
Externí odkaz:
http://arxiv.org/abs/1609.02388
Publikováno v:
MNRAS, 2012, 422, p.1546-1551
We announce the discovery of a unique combination of features in a radio source identified with the merger galaxy CGCG 292-057. The radio galaxy both exhibits a highly complex, X-like structure and shows signs of recurrent activity in the form of dou
Externí odkaz:
http://arxiv.org/abs/1203.0538
Autor:
Reed, M. D., Harms, S. L., Poindexter, S., Zhou, A. -Y., Eggen, J. R., Morris, M. A., Quint, A. C., McDaniel, S., Baran, A., Dolez, N., Kawaler, S. D., Kurtz, D. W., Moskalik, P., Riddle, R., Zola, S., Ostensen, R. H., Solheim, J. -E., Kepler, S. O., Costa, A. F. M., Provencal, J. L., Mullally, F., Winget, D. W., Vuckovic, M., Crowe, R., Terry, D., Avila, R., Berkey, B., Stewart, S., Bodnarik, J., Bolton, D., Binder, P. -M., Sekiguchi, K., Sullivan, D. J., Kim, S. -L., Chen, W. -P., Chen, C. -W., Lin, H. -C., Jian, X. -J., Wu, H., Gou, J. -P., Liu, Z., Leibowitz, E., Lipkin, Y., Akan, C., Cakirli, O., Janulis, R., Pretorius, R., Ogloza, W., Stachowski, G., Paparo, M., Szabo, R., Csubry, Z., Zsuffa, D., Silvotti, R., Marinoni, S., Bruni, I., Vauclair, G., Chevreton, M., Matthews, J. M., Cameron, C., Pablo, H.
KPD 1930+2752 is a short-period pulsating subdwarf B (sdB) star. It is also an ellipsoidal variable with a known binary period just over two hours. The companion is most likely a white dwarf and the total mass of the system is close to the Chandresak
Externí odkaz:
http://arxiv.org/abs/1011.0387
Autor:
Pribulla, T., Rucinski, S. M., Blake, R. M., Lu, W., Thomson, J. R., DeBond, H., Karmo, T., de Ridder, A., Ogloza, W., Stachowski, G., Siwak, M.
Radial-velocity measurements and sine-curve fits to the orbital radial velocity variations are presented for the last eight close binary systems analyzed the same way as in the previous papers of this series: QX And, DY Cet, MR Del, HI Dra, DD Mon, V
Externí odkaz:
http://arxiv.org/abs/0812.1313