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Table 5.
Equivalent widths of prominent emission lines in Å for the high-state spectra of Figs. 1–5.
| Name | Date | Hδ | Hγ | HeII | Hβ | HeII | HeI | Hα | |
|---|---|---|---|---|---|---|---|---|---|
| 4686 | 5411 | 5876 | |||||||
| 0154–59 | 23 Aug 93 | 103.1 | 86.5 | 81.6 | 103.9 | 11.9 | 17.2 | 87.8 | |
| 17 Dec 93 | 111.6 | 102.5 | 78.5 | 99.6 | 15.1 | 20.6 | 89.4 | ||
| 24 Nov 95 | 105.2 | 100.5 | 89.7 | 113.7 | 12.7 | 23.5 | 103.7 | ||
| 0600–27 | 16 Nov 95 | 45.7 | 57.8 | 47.7 | 55.6 | 6.7 | 17.7 | 62.3 | |
| 0859+05 | 10 Jan 03 | 27.1 | 23.3 | 20.2 | 33.9 | 4.3 | 9.5 | 33.2 | |
| 0953+05 | 6/7 Feb 95 | b | 11.2 | 11.4 | 3.4 | 13.0 | 1.0 | 3.8 | 12.7 |
| f | 48.1 | 50.3 | 20.3 | 69.4 | 2.9 | 31.2 | 80.0 | ||
| 1002–19 | 24 Dec 92 | 12.8 | 9.0 | 15.9 | 17.0 | 3.4 | 2.8 | 25.1 | |
| 1 Mar 97 | b | 11.9 | 17.7 | 15.7 | 25.5 | 3.3 | 9.0 | 35.8 | |
| f | 32.6 | 47.9 | 50.7 | 47.9 | 9.9 | 13.0 | 68.4 |
Notes. The letters b and f refer to the bright and faint orbital phase intervals, respectively.
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