Doppler Tomography of the Circumstellar Disk of the Be Star <i>κ</i> Draconis
<inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mi>κ</mi></semantics></math></inline-formula> Draconis is a binary system with a classical Be star as the primary component. Its emission-line spectrum consists of hydrogen lines, notably the H<inline-formu...
I tiakina i:
| Ngā kaituhi matua: | , , , , |
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| Hōputu: | Artigo |
| Reo: | Inglês |
| I whakaputaina: |
MDPI AG
2024-05-01
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| Rangatū: | Galaxies |
| Ngā marau: | |
| Urunga tuihono: | https://www.mdpi.com/2075-4434/12/3/23 |
| Ngā Tūtohu: |
Kāore He Tūtohu, Me noho koe te mea tuatahi ki te tūtohu i tēnei pūkete!
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