Zobrazeno 1 - 10
of 30
pro vyhledávání: '"W. Verschueren"'
Publikováno v:
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The accuracy with which radial velocities of early-type stars can be measured is limited in practice by the existence of asymmetrical dierences between object and template spectrum, constituting \spectrum mismatch". Our studies of the magnitude of sp
Publikováno v:
International Astronomical Union Colloquium. 170:108-112
We present the first results of a long-term study to increase the external accuracy of (relative and absolute) radial velocities of early-type stars below the 1 km/s level. The accuracy suffers mainly from important systematic errors caused by intrin
Autor:
M. De Bruyn, G. Van Lommen, W. J. Janssens, Jan Verrelst, M. Schroven, J. E. Leysen, W. Verschueren
Publikováno v:
ChemInform. 27
Publikováno v:
Astrophysics and Space Science. 170:245-250
We present a brief status report on our ongoing extensive and detailed Walraven photometric observations of the young stellar cluster NGC 2244 in the Rosette Nebula. The observational and reduction procedure is described together with the first resul
Autor:
M. David, W. Verschueren
Publikováno v:
Astronomy and astrophysics: supplement series
ResearcherID
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Owing to the typical morphology of spectra of early-type stars, random errors play a much more impor- tant role in the derivation of their radial velocities than in the case of late-type spectra. We derive a generalised lower bound of the random erro
Autor:
Anthony G. A. Brown, W. Verschueren, E. de Geus, P. T. de Zeeuw, H. Hensberge, M. David, R. S. Le Poole
Publikováno v:
Publications of the Astronomical Society of the Pacific. 109:868
This is the first paper in a series in which we study the kinematical structure and dynamical evolution of OB associations and young stellar clusters. By means of high-resolution high-S/N spectroscopic observations, we aim at obtaining accurate stell
Autor:
W. Verschueren, D. K. Callebaut
Publikováno v:
Astrophysics and Space Science. 137:257-266
We present an attempt for an extension of the modified Boltzmann model, which was introduced by Callebautet al. (1982) as an improvement of the polytropic models, to the case of chemically-heterogeneous stars in equilibrium, containing H and He, by p
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Publikováno v:
ResearcherID
Measuring accurate radial velocities of rotating early-type (O-B-A) stars using cross-correlation techniques is hampered by the fact that object-template spectrum mismatch causes systematic errors that do not cancel out suciently in these spectra. Th
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Akademický článek
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