Copy the page URI to the clipboard
Steele, I. A.; Negueruela, I. and Clark, J. S.
(1999).
DOI: https://doi.org/10.1051/aas:1999478
Abstract
We present a sample of 58 Be stars containing objects of spectral types O9 to B8.5 and luminosity classes III to V. We have obtained 3670 – 5070 Å spectra of the sample which are used to derive spectral types and rotational velocities. We discuss the distribution of spectral types and rotational velocities obtained and conclude that there are no significant selection effects in our sample.
Viewing alternatives
Download history
Metrics
Public Attention
Altmetrics from AltmetricNumber of Citations
Citations from DimensionsItem Actions
Export
About
- Item ORO ID
- 17840
- Item Type
- Journal Item
- ISSN
- 1432-0746
- Keywords
- emission-line stars; Be stars; fundamental parameters; rotation stars
- Academic Unit or School
-
Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM) - Copyright Holders
- © 1999 ESO
- Related URLs
- Depositing User
- Users 9108 not found.