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10830 A He I observations of 455 stars
A comparison with K line, X-ray and other data, of 10830 A equivalentwidths (EW) measurements in 890 image tube spectra of 455 stars showsthat for the case of G stars, the EW correlates well with K lineintensity. Good correlation is also found between 10830 A EW and softX-ray fluxes, confirming the excitation of the line by coronal softX-rays, which can serve as a measure of coronal emission. It is alsofound that, in contradiction to published models, 10830 A is weak orabsent in O, B and A stars, and is absent in F and M supergiants.Moderate to high 10830 A EW is frequent in F and M dwarfs, G and Ksupergiants, and class K3 III. The 58 stars whose 10830 A EW was foundto be of 300 A or more should be relatively intense X-ray emitters.Almost all RS CVn stars show strong 10830 A absorption, and T Tauristars show both absorption and emission.
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| Сазвежђа: | Змија |
| Ректацензија: | 16h15m51.81s |
| Deклинација: | +03°04'05.7" |
| Apparent магнитуда: | 8.937 |
| Даљина: | 320.513 parsecs |
| Proper motion RA: | -16.6 |
| Proper motion Dec: | -9.8 |
| B-T magnitude: | 10.436 |
| V-T magnitude: | 9.061 |
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