Zobrazeno 1 - 10
of 120
pro vyhledávání: '"W. Pych"'
Autor:
M Rozyczka, I B Thompson, A Dotter, B Mazur, W Narloch, W Pych, K G Hełminiak, A Moharana, Y Beletsky, G S Burley, J L Marshall, N Morrell, D Osip, S A Shectman, R Bernstein, B Pilecki, B Zgirski
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 517:2485-2501
We use photometric and spectroscopic observations of four detached eclipsing binaries in the globular cluster NGC 3201 to derive masses, radii, and luminosities of the component stars. Spanning across almost three magnitudes in the colour–magnitude
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b6a51172bfaa12ceaad45b32c8382bc1
https://doi.org/10.1093/mnras/stac2751
https://doi.org/10.1093/mnras/stac2751
Akademický článek
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Publikováno v:
Monthly Notices of the Royal Astronomical Society. 471:1446-1467
We derive relative proper motions of stars in the fields of the globular clusters M12, NGC 6362, M4, M55, M22, NGC 6752, NGC 3201, M30, M10, NGC 362, M5, and 47 Tucanae based on data collected between 1997 and 2015 with the 1-m Swope telescope of Las
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ac755383c60089db7bb9f328066a3d55
https://doi.org/10.1093/mnras/stx1637
https://doi.org/10.1093/mnras/stx1637
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 463:3290-3304
We present the capabilities of our new code for obtaining Doppler maps implementing the maximum likelihood approach. As test data, we used observations of the dwarf nova V2051 Ophiuchi. The system was observed in quiescence at least 16 d before the o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b87089fcb9a7b19165144596c81fd670
https://doi.org/10.1093/mnras/stw2139
https://doi.org/10.1093/mnras/stw2139
Autor:
C. Hu, Magdalena Krupa, Rupal Basak, Krzysztof Hryniewicz, Bei You, Maciej Bilicki, Jian-Min Wang, Bozena Czerny, Justyna Średzińska, T. P. Adhikari, W. Pych, Agnieszka Kurcz, Paola Marziani
Publikováno v:
Astronomy & Astrophysics (0004-6361)
Astronomy & Astrophysics (0004-6361), 601, A32
Astronomy & Astrophysics (0004-6361), 601, A32
The Mg II emission line is visible in the optical band for intermediate redshift quasars (0.4 < z < 1.6) and it is thus an extremely important tool to measure the black hole mass and to understand the structure of the Broad Line Region. We aim to det
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d58d71161f8ae0ae8e5cb8e5187b4bde
http://hdl.handle.net/20.500.12386/27189
http://hdl.handle.net/20.500.12386/27189
Akademický článek
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Autor:
R. Dymock, F. Manzini, S. Boroumand, Stephen M. Slivan, Robert D. Stephens, R. A. Koff, Greg Bolt, M. Fagas, R. Roy, Michael Fauerbach, Brian D. Warner, Josef Ďurech, Margaret Pan, A. Marciniak, M. Crow, Angel F. Lopez, Mikko Kaasalainen, Merideth Frey, Frederick Pilcher, Rita Pacheco, Thomas Bennett, S. Fauvaud, L. Crespo da Silva, C. Bembrick, W. Pych, Donald P. Pray, R. Crippa, Raoul Behrend, R. Poncy, S. Sposetti, Jérôme Berthier, T. Kwiatkowski, Marek Wolf, G. Santacana, R. Durkee, D. Jardine, Krzysztof Kamiński, Tadeusz Michalowski, W. H. Allen, Rui Soles Gonçalves, L. Bernasconi, R. Hirsch
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2007, 465, pp.331-337. ⟨10.1051/0004-6361:20066347⟩
Astronomy and Astrophysics-A&A, 2007, 465, pp.331-337. ⟨10.1051/0004-6361:20066347⟩
International audience; Aims:We present physical models of ten asteroids obtained by means of lightcurve inversion. A substantial part of the photometric data was observed by amateur astronomers. We emphasize the importance of a coordinated network o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::db87060f96dc8c4c68c527040444186c
https://doi.org/10.1051/0004-6361:20066347
https://doi.org/10.1051/0004-6361:20066347
Autor:
Michal Siwak, Theodor Pribulla, Wenxian Lu, Slavek M. Rucinski, W. Pych, George Conidis, Stefan W. Mochnacki, Heide DeBond, J. R. Thomson, Waldemar Ogloza, R. M. Blake
Publikováno v:
The Astronomical Journal. 132:769-780
Radial-velocity measurements and sine-curve fits to the orbital radial velocity variations are presented for ten close binary systems: DU Boo, ET Boo, TX Cnc, V1073 Cyg, HL Dra, AK Her, VW LMi, V566 Oph, TV UMi and AG Vir. By this contribution, the D
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bd5a71b9a019832aaa941ce8f6594ba0
https://doi.org/10.1086/505536
https://doi.org/10.1086/505536
Autor:
M. Mikolajewski, T. Tomov, M. Hajduk, M. Cikala, J. Osiwala, C. Galan, A. Zajczyk, D. Kolev, I. Iliev, P. Marrese, U. Munari, T. Zwitter, G. Galazutdinov, F. Musaev, A. Bondar, L. Georgiev, C. T. Bolton, R. M. Blake, W. Pych
Publikováno v:
Astrophysics and Space Science. 296:451-455
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::12a5976e67ef2c78f6845a256faa8521
https://doi.org/10.1007/s10509-005-4878-0
https://doi.org/10.1007/s10509-005-4878-0
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.