Reference : Périodicité de HD 10783
Scientific journals : Article
Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics
http://hdl.handle.net/2268/41106
Périodicité de HD 10783
French
Renson, Pierre mailto [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Evol. et stabilité des étoiles et des amas d'étoiles (ESEA) >]
1965
Bulletin de la Société Royale des Sciences de Liège
Société Royale des Sciences de Liège
34
118-122
Yes
International
0037-9565
Liège
Belgium
[en] The radial velocity of the magnetic star HD 10783 is shown (fig.2) to vary with the period of the luminosity and magnetic variations. The plot of the magnetic field intensity as a function of the phase (fig.1) gives an asymmetrical curve, which, except for the sign, resembles the luminosity curve, as in other periodic magnetic variables; but the coincidence of the phases remains doubtful. The velocity varies much more rapidly just before the sharper extremum of the magnetic field.
Researchers ; Students
http://hdl.handle.net/2268/41106

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