On the nature of rapidly rotating single evolved stars
We present an analysis of the nature of the rapidly rotating, apparently single giant based on rotational and radial velocity measurements carried out by the CORAVEL spectrometers. From the analyzed sample, composed of 2010 spectroscopic, apparently single, evolved stars of luminosity classes IV, II...
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| Principais autores: | , , |
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| Formato: | article |
| Idioma: | English |
| Publicado: |
American Astronomical Society
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| Assuntos: | |
| Acceso en liña: | https://repositorio.ufrn.br/jspui/handle/123456789/29085 http://dx.doi.org/10.1088/0004-637X/801/1/54 |
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