| タイトル | The discovery of nonthermal radio emission from magnetic Bp-Ap stars |
| 著者（英） | Drake, Stephen A.; Churchwell, E.; Bieging, J. H.; Abbott, David C.; Bastian, T. S. |
| 著者所属（英） | Joint Inst. for Lab. Astrophysics|California Univ.|Colorado Univ.|Wisconsin Univ. |
| 発行日 | 1987-11-15 |
| 言語 | eng |
| 内容記述 | In a VLA survey of chemically peculiar B- and A-type stars with strong magnetic fields, five of the 34 stars observed have been identified as 6 cm continuum sources. Three of the detections are helium-strong early Bp stars (Sigma Ori E, HR 1890, and Delta Ori C), and two are helium weak, silicon-strong stars with spectral types near A0p (IQ Aur = HD 34452, Babcock's star = HD 215441). The 6 cm luminosities L6 (ergs/s Hz) range from log L6 = 16.2 to 17.9, somewhat less than the OB supergiants and W-R stars. Three-frequency observations indicate that the helium-strong Bp stars are variable nonthermal sources. |
| NASA分類 | ASTROPHYSICS |
| レポートNO | 88A19106 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/373660 |
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