Rotation-Activity Connections in Main Sequence Binaries
We have studied transition-region (NV + SilV + CIV) and chromospheric (MgII) emission observed with IUE (Vilhu and Rucinski, 1982; Rucinski and Vilhu, 1982; Ayres et al., 1981) together with coronal (soft X-ray) emission observed with the Einstein satellite (Cruddace and Dupree, 1982; Walter, 1982)...
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| Veröffentlicht in: | International Astronomical Union Colloquium 1983, Vol.71, p.475-477 |
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| container_title | International Astronomical Union Colloquium |
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| creator | Vilhu, O. Rucinski, S.M. |
| description | We have studied transition-region (NV + SilV + CIV) and chromospheric (MgII) emission observed with IUE (Vilhu and Rucinski, 1982; Rucinski and Vilhu, 1982; Ayres et al., 1981) together with coronal (soft X-ray) emission observed with the Einstein satellite (Cruddace and Dupree, 1982; Walter, 1982) for contact (W UMa) and detached main sequence binaries. The components are main sequence stars (or near ms) and rapid rotators due to spin-orbit coupling. They can thus be expected to give information of dynamo-processes in rapid rotators, although the binary effects clearly produce extra complications in this discussion. |
| doi_str_mv | 10.1017/S0252921100096512 |
| format | Article |
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The components are main sequence stars (or near ms) and rapid rotators due to spin-orbit coupling. They can thus be expected to give information of dynamo-processes in rapid rotators, although the binary effects clearly produce extra complications in this discussion.</abstract><doi>10.1017/S0252921100096512</doi><tpages>3</tpages><oa>free_for_read</oa></addata></record> |
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| ispartof | International Astronomical Union Colloquium, 1983, Vol.71, p.475-477 |
| issn | 0252-9211 |
| language | eng |
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| source | Alma/SFX Local Collection |
| title | Rotation-Activity Connections in Main Sequence Binaries |
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