Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Observatory of Helsinki
University of Helsinki
Observatory, University of Helsinki
Observatory University of Helsinki
Observatory, PO Box 14, FIN-00014 University of Helsinki, Finland
University of Helsinki, Helsinki, Finland
Helsinki, University, Observatory, Finland
Univ.Helsinki
Observatory, P.O. Box 14, FIN-00014 Helsinki, Finland; INTEGRAL Science Data Center, Chemin d'Écogia 16, CH-1290 Versoix, Switzerland
Helsinki, University, Observatory, Helsinki, Finland
Observatory, P.O.Box 14, Tähtitorninmäki, Fi-00014 University of Helsinki, Finland
Helsinki Univ., Observatory, Finland
Observatory, University of Helsinki, Finland
Joint Institute for Laboratory Astrophysics, Boulder, CO
Colorado Univ., Boulder.
Observatory, University of Helsinki, P.O. Box 14, FIN-00014, Helsinki, Finland
C.E. Saclay, D.A.P.N.I.A. Service d'Astrophysique, 91191 Gif sur Yvette FranceO.VilhuObservatory, Box 14, FIN-00014 University of Helsinki, FinlandP.WallynJet Propulsion Laboratory, 169-327, California Institute of Technology, 4800 Oak Grove Dr., Pasadena, California 91109S.CorbelDowns Laboratory, 220-47, California Institute of Technology, Pasadena, California 91125
Helsinki, University, Helsinki, Finland
Helsinki University
Observatory and Astrophysics Laboratory, P.O. Box 14, FIN-00014 University of Helsinki, Finland
Helsinki Univ. Observatory, Finland
Helsinki Univ., Finland.
Akademiia Nauk SSSR, Astronomicheskii Sovet, Moscow, USSR; Astrophysical Observatory, Helsinki, Finland
Observatory, University ofHelsinki, Finland
Observatory and Astrophysics Laboratory, Box 14, FIN-00014 Helsinki, Finland
Crimean Astrophysical Lab., USSR
Observatory, P.O. Box 14, FIN-00014 University of Helsinki, Finland
Observatory, Helsinki University, Helsinki, Finland
Observatory and Astrophysics Laboratory, University of Helsinki
Joint Institute for Laboratory Astrophy
"Surface imaging of late-type contact binaries : Hα -emission in AE Phoenicis and YY Eridani"
31.4 day periodicity in Cyg X-3 ASM-data: evidence for a tertiary body or precessing disc ?
A DOR in '94
A new possible evolutionary model for AM Herculis systems.
A new ROSAT discovered polar near the lower period limit: RX J1015.5+0904 in Leonis
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