On the Optical Spectrum of Mu Cephei
High resolution spectra of M-type supergiant μ Cep are analyzed. The movements in the atmosphere of this star are highly supersonic and variable with depth. The lines forming in deeper layers show the widths corresponding to 30 kms−1. The lines forming in outer layers are much wider, 50 kms−1. At th...
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De Gruyter
2010-12-01
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| Series: | Open Astronomy |
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| Online Access: | https://doi.org/10.1515/astro-2017-0418 |
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Article |
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doaj-68f11d70da9b442898bb0eeabf71b84c2021-09-06T19:40:14ZengDe GruyterOpen Astronomy2543-63762010-12-01193-414715510.1515/astro-2017-0418astro-2017-0418On the Optical Spectrum of Mu CepheiKipper Tõnu0Tartu Observatory, Tõravere, 61602, EstoniaHigh resolution spectra of M-type supergiant μ Cep are analyzed. The movements in the atmosphere of this star are highly supersonic and variable with depth. The lines forming in deeper layers show the widths corresponding to 30 kms−1. The lines forming in outer layers are much wider, 50 kms−1. At the same time, the microturbulent velocity (ξt) is low, from 4.0 to 4.5 kms−1. The atmosphere of μ Cep is slightly metal deficient with [Fe/H]≈-0.4.https://doi.org/10.1515/astro-2017-0418starsatmospheres starsindividualμ cep |
| collection |
DOAJ |
| language |
English |
| format |
Article |
| sources |
DOAJ |
| author |
Kipper Tõnu |
| spellingShingle |
Kipper Tõnu On the Optical Spectrum of Mu Cephei Open Astronomy stars atmospheres stars individual μ cep |
| author_facet |
Kipper Tõnu |
| author_sort |
Kipper Tõnu |
| title |
On the Optical Spectrum of Mu Cephei |
| title_short |
On the Optical Spectrum of Mu Cephei |
| title_full |
On the Optical Spectrum of Mu Cephei |
| title_fullStr |
On the Optical Spectrum of Mu Cephei |
| title_full_unstemmed |
On the Optical Spectrum of Mu Cephei |
| title_sort |
on the optical spectrum of mu cephei |
| publisher |
De Gruyter |
| series |
Open Astronomy |
| issn |
2543-6376 |
| publishDate |
2010-12-01 |
| description |
High resolution spectra of M-type supergiant μ Cep are analyzed. The movements in the atmosphere of this star are highly supersonic and variable with depth. The lines forming in deeper layers show the widths corresponding to 30 kms−1. The lines forming in outer layers are much wider, 50 kms−1. At the same time, the microturbulent velocity (ξt) is low, from 4.0 to 4.5 kms−1. The atmosphere of μ Cep is slightly metal deficient with [Fe/H]≈-0.4. |
| topic |
stars atmospheres stars individual μ cep |
| url |
https://doi.org/10.1515/astro-2017-0418 |
| work_keys_str_mv |
AT kippertonu ontheopticalspectrumofmucephei |
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