You are here:
| 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  [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 | |
| 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 |
There is no file associated with this reference.
All documents in ORBi are protected by a user license.
