Table 1
Observed spectral lines in π Aquarii and their variations.
He I | Fe II | Balmer lines | Other lines | ||||
---|---|---|---|---|---|---|---|
Line | Description | Line | Description | Line | Description | Line | Description |
4388 | ♦ | 4233 | ◯ | Hδ 4102 | ▴ | O II 4254 (?) | ♦ |
4471 | ♦ | 4549 (a) | ⊗ | Hγ 4340 | ▴ | O II 4417 | ♦ |
4713 | ♦ | 4584 | ◯ | H/β 4861 | ▴ | Mg II 4481 | ♦ |
4921 | ♦ | 4629 | ⊗ | Hα 6563 | •,▴ | Si III 4552 (a) | ⊗ |
5015 (a) | • | 4667 | ⊗ | Si III 4567 | ⊗ | ||
5047 | ♦ | 5018 (a) | • | C III/O II 4650 (?) | ♦ | ||
5875 | • | 5169 | ◯ | Ti I/O II 4675 (?) | ♦ | ||
6678 | ∘ | 5198 | ◯ | Si II 6347 (a) | ⊗ | ||
7065 | ∘ | 5235 | ◯ | Si II 6371 (a) | ⊗ | ||
5276 | ◯ | ||||||
5316 | ◯ | ||||||
5363 | ◯ | ||||||
6249 | ⊗ | ||||||
6389 (a) | ⊗ | ||||||
6385 | ⊗ |
Notes. (?)Uncertainty about the element. (a)Overlapping lines. Description of each line: ⊗ No signal or very weak transition between emission and absorption lines. • DPS emission with variations over the years. ♦ Absorption line with some variations. ∘ DPS in early years (2001–2014), disappearing and reforming in later years. ▴ Transition between shell-type and DPS profiles. ◯ DPS formation in final years (2014–2024).
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