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A P Cygni Profile for the He 10830 A line of CI Cyg in Eclipse
Published online by Cambridge University Press: 12 April 2016
Abstract
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Infrared spectroscopic observations of CI Cyg in eclipse show a P Cygni profile for He I 10830 Å, with a wind velocity of the order of 150 km/s, not seen in hydrogen Brackett and Paschen emission lines, which are single peaked.
- Type
- Session 3. Physics of Individual Objects
- Information
- International Astronomical Union Colloquium , Volume 103: The Symbiotic Phenomenon , 1988 , pp. 193 - 195
- Copyright
- Copyright © Kluwer 1988
References
Bensammar, S., Friedjung, M., Letourneur, N., Maillard, J.P., 1987, Astron. Astrop., in pressGoogle Scholar
Bernat, A.P., Hall, D.N.B., Hinkle, K.H., Ridgway, S.T., 1979, Ap. J. (Letters), 233, L135.CrossRefGoogle Scholar
Maillard, J.P. and Michel, G., 1982, in IAU Colloquium No 92, Instrumentation for Astronomy with large Telescopes, ed. Humphries, C.M., (D. Reidel Pub.), p. 213.CrossRefGoogle Scholar
Oliversen, N.A., Anderson, C.M., Nordsieck, K.H., 1982, in IAU Colloquium No 70 The Nature of Symbiotic Stars, ed By Friedjung, M. and Viotti, R. (D. Reidel Pub), p. 153.CrossRefGoogle Scholar
Stencel, E.S., Michalitsianos, A.G., Kafatos, M., Boyarchuk, A.A., 1982, Ap. J. Letters, 253, L77.Google Scholar