Zobrazeno 1 - 10
of 225
pro vyhledávání: '"Slavek M. Rucinski"'
Autor:
Werner W. Weiss, Konstanze Zwintz, Rainer Kuschnig, Gerald Handler, Anthony F. J. Moffat, Dietrich Baade, Dominic M. Bowman, Thomas Granzer, Thomas Kallinger, Otto F. Koudelka, Catherine C. Lovekin, Coralie Neiner, Herbert Pablo, Andrzej Pigulski, Adam Popowicz, Tahina Ramiaramanantsoa, Slavek M. Rucinski, Klaus G. Strassmeier, Gregg A. Wade
Publikováno v:
Universe, Vol 7, Iss 6, p 199 (2021)
BRITE-Constellation is devoted to high-precision optical photometric monitoring of bright stars, distributed all over the Milky Way, in red and/or blue passbands. Photometry from space avoids the turbulent and absorbing terrestrial atmosphere and all
Externí odkaz:
https://doaj.org/article/ea1eaae50a7a49ed95580ffc7e659ca9
Autor:
T. Kallinger, Wade G.A, Adam Popowicz, Herbert Pablo, C. Neiner, Catherine Lovekin, Weiss W.W, Klaus G. Strassmeier, T. Ramiaramanantsoa, Otto Koudelka, Gerald Handler, Dominic M. Bowman, T. Granzer, Slavek M. Rucinski, Moffat A.F.J., D. Baade, Andrzej Pigulski, Rainer Kuschnig, K. Zwintz
Publikováno v:
Universe, Vol 7, Iss 199, p 199 (2021)
BRITE-Constellation is devoted to high-precision optical photometric monitoring of bright stars, distributed all over the Milky Way, in red and/or blue passbands. Photometry from space avoids the turbulent and absorbing terrestrial atmosphere and all
Autor:
Marek Drozdz, Diana P. Kjurkchieva, Slavek M. Rucinski, Michal Siwak, Dorota Kozieł-Wierzbowska, Ahmet Erdem, G. Stachowski, Andrzej S. Baran, Waldemar Ogloza, Dragomir Marchev, B. Zakrzewski, S. Szalankiewicz, Kosmas Gazeas, Alexios Liakos, Stanisław Zoła, J. M. Kreiner
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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::60e8ea5ccfaa03d81981feb6e06f4196
Autor:
Chris Cameron, Thomas Kallinger, Waldemar Ogloza, David B. Guenther, Jason F. Rowe, Anthony F. J. Moffat, Michal Siwak, Jaymie M. Matthews, Slavek M. Rucinski, Rainer Kuschnig, Dimitar Sasselov, Werner W. Weiss
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 478:758-783
This is the final photometric study of TW Hya based on new MOST satellite observations. During 2014 and 2017 the light curves showed stable 3.75 and 3.69 d quasi-periodic oscillations, respectively. Both values appear to be closely related with the s
Autor:
Slavek M. Rucinski, M. Müllner, A. F. J. Moffat, Daniel R. Reese, Werner W. Weiss, Remko Stuik, Gerald Handler, Rainer Kuschnig, Eric E. Mamajek, Samuel N. Mellon, John I. Bailey, B. Lomberg, Tristan Guillot, Matthew A. Kenworthy, G. J. J. Talens, Andrzej Pigulski, Michael J. Ireland, Coralie Neiner, L. Abe, Steven M. Crawford, Gregg A. Wade, S. Zieba, Adam Popowicz, Konstanze Zwintz
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 627, pp.A28. ⟨10.1051/0004-6361/201834744⟩
Astronomy and Astrophysics (0004-6361), 627, A28
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 627, pp.A28. ⟨10.1051/0004-6361/201834744⟩
Astronomy and Astrophysics (0004-6361), 627, A28
Exoplanet properties crucially depend on their host stars' parameters. In case the exoplanet host star shows pulsations, asteroseismology can be used for an improved description of the stellar parameters. We aim to revisit the pulsational properties
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fed1acf3d047a77d9f2ec35adb934dca
http://arxiv.org/abs/1905.12545
http://arxiv.org/abs/1905.12545
Autor:
Gregor Rauw, Adam Popowicz, Coralie Neiner, Werner W. Weiss, Slavek M. Rucinski, Herbert Pablo, Yaël Nazé, A. F. J. Moffat, Françoise Raucq, Konstanze Zwintz, Alexandre David-Uraz, Gregg A. Wade, Eric Gosset, Andrzej Pigulski, Gerald Handler
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 621, pp.A15. ⟨10.1051/0004-6361/201833594⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 621, pp.A15. ⟨10.1051/0004-6361/201833594⟩
HD149404 is an evolved non-eclipsing O-star binary that has previously undergone a Roche lobe overflow interaction. Understanding some key properties of the system requires a determination of the orbital inclination and of the dimensions of the compo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::32b32951a4d3bc041000a8d5ffe716ef
https://hal.archives-ouvertes.fr/hal-02323438
https://hal.archives-ouvertes.fr/hal-02323438
Autor:
Rainer Kuschnig, Radosław Smolec, Ernst Paunzen, Stéphane Mathis, Slavek M. Rucinski, Evelyne Alecian, C. Neiner, Adam Popowicz, Andrzej Pigulski, Jim Fuller, Gerald Handler, Werner W. Weiss, A. F. J. Moffat, J.-B. Le Bouquin, Gregg A. Wade, Konstanze Zwintz, Matt Shultz, Herbert Pablo
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2019, 488 (1), pp.64-77. ⟨10.1093/mnras/stz1661⟩
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2019, 488 (1), pp.64-77. ⟨10.1093/mnras/stz1661⟩
Monthly Notices of the Royal Astronomical Society, 2019, 488 (1), pp.64-77. ⟨10.1093/mnras/stz1661⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2019, 488 (1), pp.64-77. ⟨10.1093/mnras/stz1661⟩
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2019, 488 (1), pp.64-77. ⟨10.1093/mnras/stz1661⟩
Monthly Notices of the Royal Astronomical Society, 2019, 488 (1), pp.64-77. ⟨10.1093/mnras/stz1661⟩
$\varepsilon$ Lupi A is a binary system consisting of two main sequence early B-type stars Aa and Ab in a short period, moderately eccentric orbit. The close binary pair is the only doubly-magnetic massive binary currently known. Using photometric da
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5fad649ca84b9de17dabda9ab062053d
http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-394700
http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-394700
Autor:
G. Whittaker, Gerald Handler, Slavek M. Rucinski, A. F. J. Moffat, Andrzej Pigulski, Adam Popowicz, Konstanze Zwintz, M. Rybicka, Herbert Pablo, Werner W. Weiss, E. Zocłońska, Cordell Grant, Tahina Ramiaramanantsoa, Gregg A. Wade, Rainer Kuschnig
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 464:2249-2258
We report a simultaneous ground and space-based photometric study of the Beta Cephei star Nu Eridani. Half a year of observations have been obtained by four of the five satellites constituting BRITE-Constellation, supplemented with ground-based photo
Autor:
Jason F. Rowe, Werner W. Weiss, Waldemar Ogloza, Jaymie M. Matthews, Anthony F. J. Moffat, Dimitar Sasselov, Slavek M. Rucinski, David B. Guenther, Rainer Kuschnig, Michal Siwak, C. Cameron
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 456:3972-3984
Results of the time variability monitoring of the two classical T Tauri stars, RU Lup and IM Lup, are presented. Three photometric data sets were utilised: (1) simultaneous (same field) MOST satellite observations over four weeks in each of the years
Autor:
Raphael Maltais-Tariant, Judit Sturmann, Chris Farrington, Nic Scott, Anatoly S. Miroshnichenko, Anthony F. J. Moffat, Sergey Zharikov, Dimitar Sasselov, T. ten Brummelaar, Jason F. Rowe, Deepak Raghavan, Werner W. Weiss, Slavek M. Rucinski, Tahina Ramiaramanantsoa, Rainer Kuschnig, Stephen T. Ridgway, C. Cameron, Nils H. Turner, Harold A. McAlister, Jaymie M. Matthews, Norm Vargas, Jeremy Jones, Douglas R. Gies, Laszlo Sturmann, Noel D. Richardson, David O'Brien, Hideyuki Saio, Joshua D. Thomas, Herbert Pablo, Tabetha S. Boyajian, Kathryn Gordon, Emily J. Aldoretta, Étienne Artigau, David B. Guenther, Rachel A. Matson, Gail Schaefer, Nicole St-Louis
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 455:244-257
MWC 314 is a bright candidate luminous blue variable that resides in a fairly close binary system, with an orbital period of 60.753$\pm$0.003 d. We observed MWC 314 with a combination of optical spectroscopy, broad-band ground- and space-based photom