Zobrazeno 1 - 10
of 24
pro vyhledávání: '"J, Denoyelle"'
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Publikováno v:
Parasitology
Parasitology, Cambridge University Press (CUP), 2018, 145 (6), pp.775-782. ⟨10.1017/S0031182017001330⟩
Parasitology, Cambridge University Press (CUP), 2018, 145 (6), pp.775-782. ⟨10.1017/S0031182017001330⟩
Vertically transmitted parasites (VTPs) such asWolbachiaare expected not only to minimize the damage they inflict on their hosts, but also to protect their hosts against the damaging effects of coinfecting parasites. By modifying the fitness costs of
Autor:
F Rufener, R. Polfliet, C. Waelkens, J. Cuypers, D. Heynderickx, K. Degryse, K. Van Den Abeele, Patricia Lampens, Stefaan Poedts, Paul Smeyers, J. Denoyelle
Publikováno v:
Astrophysics and Space Science. 169:109-111
Precise photometric observations of stars in the double cluster h and Ξ Persei reveal a large spread in the colours and magnitudes of the upper Main-Sequence; half of the stars are variables that are Be stars or related stars. The reported age diffe
Publikováno v:
Pulsation, Rotation and Mass Loss in Early-Type Stars ISBN: 9780792330455
The double cluster h and χ Persei is one of the richest clusters containing early-B stars, and therefore is important for observational and theoretical studies on the fundamental parameters of massive stars. The colour-magnitude diagram of the doubl
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ca4a2882f6c9f2fa32ac26083e69e279
https://doi.org/10.1007/978-94-011-1030-3_42
https://doi.org/10.1007/978-94-011-1030-3_42
Publikováno v:
Symposium - International Astronomical Union. 162:151-152
The double cluster h andxPersei is one of the richest clusters containing early-B stars, and therefore is important for observational and theoretical studies on the fundamental parameters of massive stars. The colour-magnitude diagram of the double c
Publikováno v:
Astrophysics and Space Science. 37:221-233
The behavior ofp-modes of high degree and high order in the homogeneous compressilbe model is examined. The second-order differential equation of Pekeris is used to construct asymptotic expansions near the centre and near the surface, which are singu
Publikováno v:
International Astronomical Union Colloquium. 92:505-508
The double cluster h and χ Persei has since long been known to be rich in Be stars (Trumpler, 1926). It belongs to an age group in which various types of variable stars occur (Mermilliod, 1981). Other clusters of this age group are NGC 3293, the clu
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Ivan R. King, A. N. Argue, null Willstrop, A. W. J. Cousins, J. Denoyelle, A. G. Velghe, P. S. The, A. N. Argne, E. W. Miller, Ch. R. Tolbert, F. Rufener, H. R. Butcher, R. M. West, R. D. Cannon, M. F. McCarthy, E. Peytremann
Publikováno v:
Transactions of the International Astronomical Union ISBN: 9789401012591
The most widely used photometric system, photographic B and V, has serious systematic problems that are not generally recognized. The photographic sensitivity bands do not match well with the corresponding photoelectric sensitivity bands; and as a re
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::fc0d6fd861275c23a08699d2354c5c01
https://doi.org/10.1007/978-94-010-1257-7_21
https://doi.org/10.1007/978-94-010-1257-7_21