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Neutral oxygen in herbig Ae stars
Published online by Cambridge University Press: 04 August 2017
Abstract
In stars with dense envelopes such as classical Be and T Tauri stars, the near infrared lines of OI have been observed: λ 8446 Å in emission, λ 7772 Å in absorption or in emission (e.g. Polidan and Peters, 1976; Herbig and Soderblom, 1980). In Herbig stars, only low resolution (2-7 Å) material is available on a few objects (Shanin et al. 1975; Andrillat and Swings, 1976).
- Type
- Bipolar Flows, Jets and Protostars
- Information
- Symposium - International Astronomical Union , Volume 122: Circumstellar Matter , 1987 , pp. 101 - 102
- Copyright
- Copyright © Reidel 1987