Hostname: page-component-586b7cd67f-gb8f7 Total loading time: 0 Render date: 2024-12-01T09:10:48.432Z Has data issue: false hasContentIssue false

Mass Loss from π Aquarii

Published online by Cambridge University Press:  14 August 2015

J.A. de Freitas Pacheco*
Affiliation:
CNPq-Observatório Nacional, Rua General Bruce, 586 - São Cristovão, Rio de Janeiro - Brasil

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.

Fe III lines from metastable states have been detected in the UV spectrum of π Aqr (HD 212571). The line profiles are asymmetric and they are probably formed in a expanding envelope. From the observed fine widths and using the Sobolev approximation we have derived a mass loss rate of about 2.5 × 10−9M y−1.

Type
VII. UV Observations and Mass Loss
Copyright
Copyright © Reidel 1982 

References

- Bruhweiler, F.C., Morgan, T.H. and van der Hucht, K.: 1978, Astrophys. J., 255, L 71.Google Scholar
- Hensberge, H.G., van den Heuvel, E.P.J., Lamers, H.I.G., Burger, M., de Loore, C., Glencross, W., Howarth, I., Willis, A.J., Wilson, R. and Menzies, J.: 1980, Astron. Astrophys., 85, 119.Google Scholar
- Lamers, H.J.G. and Rogerson, J.: 1978, Astron. Astrophys. 66, 417.Google Scholar
- Ringuelet, A., Fontenla, J.M. and Rovira, M.: 1981 - preprint.Google Scholar