Published 1982
| Version v1
Book
Mass loss from π Aquarii
Description
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 an expanding envelope. From the observed line widths and using the Sobolev approximation the author has derived a mass loss rate of about 2.5 x 10-9solar masses y-1. (Auth.)
Additional details
Publishing Information
- Publisher
- D. Reidel.
- Imprint Place
- Dordrecht, Netherlands
- ISBN
- 90-277-1366-9
- Imprint Title
- Be stars
- Imprint Pagination
- 536 p.
- Journal Issue
- no. 98
- Series
- International astronomical union symposium.
- Journal Page Range
- p. 391-392.
Conference
- Title
- Be stars.
- Dates
- 6 - 10 Apr 1981.
- Place
- Munich, Germany, F.R.
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- Netherlands
- INIS RN
- 13670528
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- EMISSION SPECTRA; IRON; MASS TRANSFER; STARS; ULTRAVIOLET SPECTRA
- Descriptors DEC
- ELEMENTS; METALS; SPECTRA; TRANSITION ELEMENTS