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Numerical Modelling and Simulation for Multi-Spacecraft Data Analysis: Approaches and Examples
Büchner, Jörg; Kuska, Jens-Peer; Wiechen, Heinz
CP stars: Photometric calibrations of luminosity using HIPPARCOS data
Jordi, C.; Luri, X.; Figueras, F. +7 more
The application of the Stromgren photometric luminosity calibrations to different types of CP stars is reexamined in the light of the new Hipparcos data. A first attempt is made to use the LM statistical parallax method - based on the maximum likelihood principle - to obtain a calibration of the absolute magnitude as a function of two Stromgren co…
Hubble Space Telescope-WFPC2/Hα Observations of the Ejected Nebula M1-67
Moffat, Anthony F. J.; Grosdidier, Yves; Acker, Agnès
We present HST-WFPC2/Hα deep images of the ejected nebula M1-67. Our data suggest that M1-67 is the imprint of a previous, slow LBV wind ejected from the central star WR124, now a WN8 star. We find evidence that the LBV wind is highly variableand anisotropic. Some dense, persisting clumps have possibly been ejected directly from the stellar surfac…
Planetary Nebulae
Cox, P.
This review summarizes spectroscopic and imaging results obtained on board the Infrared Space Observatory (ISO) on well-known planetary nebulae: the young nebula NGC 7027, and two fully evolved nearby nebulae, the Dumbbell and the Helix.
Stellar Wind Variability from IUE Spectra of Epsilon Orionis
Sapar, L.; Sapar, A.
21 IUE spectra of epsilon Ori (HD 37128), B0 supergiant, were studied to analyze variations in the profiles of the resonance lines of N V, C IV, Si IV and Si III. The largest variations in the profiles of resonance doublets of N V, C IV and Si IV are found in blue wings of the lines at velocities from --1500 to --2000 km/s, reaching in some spectr…
Mass Loss During Proto-Planetary Phase of Evolution The Case of HD 101584 = IRAS 11385-5517
Szczerba, Ryszard; Gesicki, Krzysztof
ISO Spectra of Symbiotic Stars
Vogel, M.; Schild, H.
ISOPHOT Mapping Observations of Carbon Stars
Izumiura, H.; Hashimoto, O.
Mapping observations have been made toward five carbon stars in the far-infrared using ISOPHOT, an imaging photo-polarimeter on board the Infrared Space Observatory. Cold, very extended dust shells are clearly revealed in two of them. Y CVn is surrounded by a very extended, detached dust shell, which indicates a sudden decline of the mass-loss by …
The energy distribution of Beta CrB for the specific stellar abundances
Castelli, F.
The comparison of the observed and computed energy distributions of Beta CrB has shown that a model with the specific chemical composition of the star can account for the visual energy distribution, while it is still unable to reproduce ultraviolet observations shortward of 1700 Angstroms. Furthermore, the predicted absorption of strong Fe II and …
Theory of AGB Evolution
Blöcker, Thomas