Abstract
Recent GHRS observations of the Herbig Ae star AB Aur demonstrate the presence of N V in the wind of this star. We found that models including hot (T≈140,000 K) clumps are able to reproduce the available observations and are also consistent with its X-ray emission.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Preview
Unable to display preview. Download preview PDF.
References
Catala C., Kunasz P.B., 1987, A&A, 174, 158
Catala C., Praderie F., Felenbok P., 1987, A&A, 182, 115
Mihalas D., Kunasz P., 1978, ApJ, 219, 635
Mullan D., 1984, ApJ, 283, 303
Zinnecker H., Preibisch Th., 1994 A&A 292, 152
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1998 Springer Science+Business Media Dordrecht
About this chapter
Cite this chapter
Bouret, JC., Catala, C., Simon, T. (1998). Nitrogen V in the Wind of the Pre-Main Sequence Herbig Ae Star AB Aur. In: Hubert, A.M., Jaschek, C. (eds) B[e] Stars. Astrophysics and Space Science Library, vol 233. Springer, Dordrecht. https://doi.org/10.1007/978-94-015-9014-3_8
Download citation
DOI: https://doi.org/10.1007/978-94-015-9014-3_8
Publisher Name: Springer, Dordrecht
Print ISBN: 978-90-481-5080-9
Online ISBN: 978-94-015-9014-3
eBook Packages: Springer Book Archive