Zobrazeno 1 - 10
of 21
pro vyhledávání: '"A. Budovičová"'
Autor:
Saad, S. M., Kubat, J., Korcakova, D., Koubsky, P., Skoda, P., Slechta, M., Kawka, A., Budovicova, A., Votruba, V., Sarounova, L., Nouh, M. I.
We have carried out a spectroscopic survey of several B, Be, and shell stars in optical and near-infrared regions. Line profiles of the H-alpha line and of selected Fe II and O I lines are presented.
Comment: 23 pages, 45 figures; accepted in As
Comment: 23 pages, 45 figures; accepted in As
Externí odkaz:
http://arxiv.org/abs/astro-ph/0512619
Publikováno v:
Astrophysics and Space Science. 296:169-172
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::45d8dda43b26f67d58e9eb5188fe1ae7
https://doi.org/10.1007/s10509-005-4428-9
https://doi.org/10.1007/s10509-005-4428-9
Autor:
A. Budovičová, S. Štefl, Dietrich Baade, Otmar Stahl, Andreas Kaufer, M. Maintz, Th. Rivinius
Publikováno v:
Astronomy & Astrophysics. 411:167-180
The rapid line-profile variability of the early-type and pole-on Be star ω CMa between 1996 and 2002 is characterized across the complete optical spectrum, for quiescent phases as well as for outbursts. Owing to differentand changing line-profile va
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2eb63a75e37faaf48649fcf121911b60
https://doi.org/10.1051/0004-6361:20031179
https://doi.org/10.1051/0004-6361:20031179
Publikováno v:
International Astronomical Union Colloquium. 175:240-243
Spectra of the Be star 28 CMa obtained with the HEROS echelle spectrograph in 1996 and 1997 were used to check the presence of transient periods in commonly measured scalar parameters of absorption and emission lines. Transient periods can be convinc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8b60c03e61d98cca3410804a8221d38f
https://doi.org/10.1017/s0252921100055913
https://doi.org/10.1017/s0252921100055913
Publikováno v:
Zdeněk Kopal’s Binary Star Legacy ISBN: 1402031319
oAnd is one of the most frequently observed Be stars, both in photometry and spectroscopy. It is a multiple system of at least four stars (a Be star, a close binary of spectral types B7 and B8, and an A star). For over a century, numerous observers r
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0aede50d8ade155b44cf22efbe987cd1
https://doi.org/10.1007/1-4020-3875-5_22
https://doi.org/10.1007/1-4020-3875-5_22
Autor:
Saad, S. M., Kubát, J., Korčáková, D., Koubský, P., Škoda, P., Šlechta, M., Kawka, A., Budovičová, A., Votruba, V., Šarounová, L., Nouh, M. I., Saad, S. M., Kubát, J., Korčáková, D., Koubský, P., Škoda, P., Šlechta, M., Kawka, A., Budovičová, A., Votruba, V., Šarounová, L., Nouh, M. I.
Publikováno v:
Astronomy and Astrophysics; April 2006, Vol. 450 Issue: 1 p427-430, 4p
Autor:
Štefl, S., Baade, D., Rivinius, Th., Stahl, O., Budovičová, A., Kaufer, A., Maintz, M., Štefl, S., Baade, D., Rivinius, Th., Stahl, O., Budovičová, A., Kaufer, A., Maintz, M.
Publikováno v:
Astronomy and Astrophysics; November 2003, Vol. 411 Issue: 2 p167-180, 14p
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.