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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ri-123456789-290852022-10-20T20:37:31Z On the nature of rapidly rotating single evolved stars Silva, R. Rodrigues da Martins, B. L. Canto Medeiros, José Renan de Stars: evolution Stars: rotation 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, III, II, and Ib with spectral types G and K, we classified 30 stars that presented unusual, moderate to rapid rotation. This work reports, for the first time, the presence of these abnormal rotators among subgiant, bright giant, and Ib supergiant stars. To date, this class of stars was reported only among giant stars of luminosity class III. Most of these abnormal rotators present an IRAS infrared excess, which, in principle, can be related to dust around these stars. 2020-05-28T12:36:30Z 2020-05-28T12:36:30Z 2015 article MEDEIROS, José Renan de et al. On the nature of rapidly rotating single evolved stars. Astrophysical Journal (Online), [s. l.], v. 801, p. 54, 2015. ISSN 1538-4357 versão online. DOI https://doi.org/10.1088/0004-637X/801/1/54. Disponível em: http://iopscience.iop.org/article/10.1088/0004-637X/801/1/54/meta. Acesso em: 28 maio 2020. 0004-637X (print), 1538-4357 (online) https://repositorio.ufrn.br/jspui/handle/123456789/29085 http://dx.doi.org/10.1088/0004-637X/801/1/54 en American Astronomical Society |
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English |
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Stars: evolution Stars: rotation |
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Stars: evolution Stars: rotation Silva, R. Rodrigues da Martins, B. L. Canto Medeiros, José Renan de On the nature of rapidly rotating single evolved stars |
description |
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, III, II, and Ib with spectral types G and K, we classified 30 stars that presented unusual, moderate to rapid rotation. This work reports, for the first time, the presence of these abnormal rotators among subgiant, bright giant, and Ib supergiant stars. To date, this class of stars was reported only among giant stars of luminosity class III. Most of these abnormal rotators present an IRAS infrared excess, which, in principle, can be related to dust around these stars. |
format |
article |
author |
Silva, R. Rodrigues da Martins, B. L. Canto Medeiros, José Renan de |
author_facet |
Silva, R. Rodrigues da Martins, B. L. Canto Medeiros, José Renan de |
author_sort |
Silva, R. Rodrigues da |
title |
On the nature of rapidly rotating single evolved stars |
title_short |
On the nature of rapidly rotating single evolved stars |
title_full |
On the nature of rapidly rotating single evolved stars |
title_fullStr |
On the nature of rapidly rotating single evolved stars |
title_full_unstemmed |
On the nature of rapidly rotating single evolved stars |
title_sort |
on the nature of rapidly rotating single evolved stars |
publisher |
American Astronomical Society |
publishDate |
2020 |
url |
https://repositorio.ufrn.br/jspui/handle/123456789/29085 http://dx.doi.org/10.1088/0004-637X/801/1/54 |
work_keys_str_mv |
AT silvarrodriguesda onthenatureofrapidlyrotatingsingleevolvedstars AT martinsblcanto onthenatureofrapidlyrotatingsingleevolvedstars AT medeirosjoserenande onthenatureofrapidlyrotatingsingleevolvedstars |
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1773960791104421888 |