Table 2
Observed emission lines of ISO 217.
Date | Lobe | Peak | EW | ||
λ [Å] | v [km s-1] | [Å] | |||
|
|||||
Ca II | 2008 03 22 | 8498.45 ± 0.02 | 8.4 ± 1.4 | –6.2 ± 0.3 | |
(8498.02 Å) | 2009 01 30 | 8498.22 ± 0.03 | 1.8 ± 1.5 | –2.0 ± 0.1 | |
2009 02 23 (spec 5) | 8498.39 ± 0.02 | 8.1 ± 1.3 | –6.1 ± 0.3 | ||
2009 02 23 (spec 6) | 8499.01 ± 0.02 | 29.8 ± 1.4 | –6.3 ± 0.3 | ||
2009 02 23 (spec5&6) | 8498.63 ± 0.02 | 16.4 ± 1.4 | –6.2 ± 0.3 | ||
|
|||||
[S II] | 2008 03 22 | red | 6731.75 ± 0.01 | 34.2 ± 1.2 | –4.5 ± 0.2 |
(6730.82 Å) | 2008 03 22 | blue | 6730.46 ± 0.01 | –23.0 ± 1.2 | |
2009 01 30 | red | 6731.69 ± 0.01 | 33.6 ± 1.2 | –5.3 ± 0.3 | |
2009 01 30 | blue | 6730.36 ± 0.01 | –25.7 ± 1.2 | ||
2009 02 23 | red | 6731.71 ± 0.01 | 34.8 ± 1.2 | –4.3 ± 0.2 | |
2009 02 23 | blue | 6730.54 ± 0.01 | –17.4 ± 1.2 | ||
|
|||||
[S II] | 2008 03 22 | red | 6717.35 ± 0.01 | 33.4 ± 1.2 | –2.5 ± 0.1 |
(6716.44 Å) | 2008 03 22 | blue | 6716.28 ± 0.02 | –14.1 ± 1.4 | |
2009 01 30 | red | 6717.33 ± 0.01 | 34.4 ± 1.2 | –3.4 ± 0.2 | |
2009 01 30 | blue | 6716.17 ± 0.02 | –17.5 ± 1.4 | ||
2009 02 23 | red | 6717.34 ± 0.01 | 35.0 ± 1.2 | –2.4 ± 0.1 | |
2009 02 23 | blue | 6716.16 ± 0.01 | –17.6 ± 1.2 | ||
|
|||||
[Fe II] | 2009 02 23 | 7155.21 ± 0.05 | –2.89 ± 2.1 | –1.6 ± 0.1 | |
(7155.16 Å) |
Notes. The laboratory wavelengths of the emission lines are taken from the NIST database (http://physics.nist.gov/asd3, Ralchenko et al. 2011). The error in the EW is assumed to be 5% of the determined value. The errors in the peak values (λ, v) are based on the errors in the Gaussian fit parameters. The errors in λ and v are underestimated in the case of deviations from a Gaussian shape ([S II], [Fe II]). See the text for more details.
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