No CrossRef data available.
Article contents
Near Infrared Spectra of 103 Bright Be Stars
Published online by Cambridge University Press: 23 September 2016
Extract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
We have observed 103 bright Be stars in the near infrared up to 10500 A with a dispersion of 230 and 50 A mm-1. The observations were performed with a Reticon (1024 diodes) attached to the ROUCAS spectrograph at the 193 cm telescope of the Haute Provence Observatory.
In this spectral range, the Be stars are characterized by the lines of HI (Paschen series), 0I(7772-74-75, 8446 A), CaII(8542, 8662, 8498 A), FeII(7712, 9997 A) and NI(8686-83-80, 8719-12-03, 8629 A).
On our spectra, the CaII triplet is always blended with P13, P15, P16, and only the enhancement of these lines permits to conclude to the CaII presence. The 0I 8446 A is perturbed by the Paschen lines P17 and P18 (low dispersion spectra) and P18 (high dispersion spectra). The NI 8686-83-80 A lines also perturb the P13 profile.
- Type
- III. The Circumstellar Gas
- Information
- International Astronomical Union Colloquium , Volume 92: Physics of Be Stars , August 1987 , pp. 237 - 238
- Copyright
- Copyright © Cambridge University Press 1987
References
Reference List
Andrillat, Y. & Houziaux, L. (1967). Spectres IR de quelques étoiles des premiers types entre 6500 et 8800 A. J. Obs., 50, 107.Google Scholar
Kitchin, C.R. & Meadows, A.J. (1970). The behaviour of the IR lines of OI lines. Astrophys. Space Sci., 8, 463.CrossRefGoogle Scholar
Polidan, R.S. & Peters, G.J. (1976). Spectroscopic obs. of Be stars in the near IR. IAU Syrap. n° 70. Ed. Slettebak, A., 59.Google Scholar
You have
Access