Zobrazeno 1 - 10
of 13
pro vyhledávání: '"Miroslav Plavec"'
Autor:
Miroslav Plavec, R. Hoekstra, C. De Jager, Ji⋖´ Grygar, J. Otterman, H. M. van den Dool, O. Namba, C. J. Th. Gunsing, Jean-Claude Pecker, K. K. Kwee, L. Perek, D. Callebaut, Jan Kuijpers, W. de Graaff, G. C. M. Reijnen, B. Swanenburg, N. Grevesse, J. Kleczek, P. P≙quet, A. D. Fokker, H. G. van Bueren, D. Edgar Page, R. J. van Duinen, Franco Pacini
Publikováno v:
Space Science Reviews. 21:469-483
Autor:
Miroslav Plavec
Publikováno v:
Symposium - International Astronomical Union. 70:439-444
The hypothesis that a significant fraction of Be stars are interacting binaries is discussed in general terms. The author believes that the observed Be stars are a mixture of three different types of objects. The weakest point of the single-star hypo
Autor:
Miroslav Plavec
Publikováno v:
Symposium - International Astronomical Union. 70:1-10
The early history of the studies on Be stars is reviewed. The importance of keeping in mind a basic model of a Be star is emphasized, and the binary star model is suggested as one serious possibility at least for some Be stars.
Autor:
Miroslav Plavec
Publikováno v:
Transactions of the International Astronomical Union. 15:647-667
Autor:
Miroslav Plavec
Publikováno v:
Symposium - International Astronomical Union. 51:216-259
Several groups of close binary stars are considered in an attempt to explain their present state as a consequence of a large-scale mass transfer or mass loss in the past: Algol-like semidetached binaries, some shell stars (AX Mon), some binary X-ray
Autor:
Miroslav Plavec
Publikováno v:
International Astronomical Union Colloquium. 4:132-146
When studying the axial rotation of the components of binary systems, we ask the following fundamental question: How much is axial rotation affected by the other star? In particular, is there any synchronism between the periods of axial rotation and
Autor:
Miroslav Plavec
Publikováno v:
Vistas in Astronomy. 2:994-998
Meteor showers show wide variations in many properties, for example, in hourly rate, duration, periodicity, concentration of the radiants, etc . The author believes that many, if not all, of these differences can be explained in terms of the evolutio
Autor:
Miroslav Plavec
Publikováno v:
Be and Shell Stars ISBN: 9789027707000
The hypothesis that a significant fraction of Be stars are interacting binaries is discussed in general terms. The author believes that the observed Be stars are a mixture of three different types of objects. The weakest point of the single-star hypo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::dc1ee8d7445fad42b74b08bcc7746414
https://doi.org/10.1007/978-94-010-1498-4_49
https://doi.org/10.1007/978-94-010-1498-4_49
Autor:
Miroslav Plavec
Publikováno v:
Be and Shell Stars ISBN: 9789027707000
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::040f9a19fc178430d75ebaf5c51202e1
https://doi.org/10.1007/978-94-010-1498-4_1
https://doi.org/10.1007/978-94-010-1498-4_1