Table 2
Observed emission lines of ISO 143.
Line | Slit PA | Date | Blue component | Green component | Red component | ||||||
V | FWHM | EW | V | FWHM | EW | V | FWHM | EW | |||
[deg] | [km s-1] | [km s-1] | [Å] | [km s-1] | [km s-1] | [Å] | [km s-1] | [km s-1] | [Å] | ||
|
|||||||||||
[S II] | 3.1 | 2009 01 15 | ... | ... | ... | ... | ... | ... | 40.8 | 27.3 | –0.2 |
(6716.44 Å) | 10.4 | 2008 03 19 | ... | ... | ... | ... | ... | ... | 41.9 | 28.6 | –0.2 |
42.2 | 2009 02 10 | ... | ... | ... | ... | ... | ... | 49.8 | 30.8 | –0.2 | |
|
|||||||||||
[S II] | 3.1 | 2009 01 15 | ... | ... | ... | ... | ... | ... | 44.2 | 31.7 | –0.4 |
(6730.82 Å) | 10.4 | 2008 03 19 | ... | ... | ... | ... | ... | ... | 44.5 | 26.7 | –0.5 |
42.2 | 2009 02 10 | ... | ... | ... | ... | ... | ... | 44.6 | 32.5 | –0.4 | |
|
|||||||||||
He I | 3.1 | 2009 01 15 | ... | ... | ... | –0.5 | 34.5 | –0.4 | ... | ... | ... |
(7065.19 Å) | 10.4 | 2008 03 19 | ... | ... | ... | –2.3 | 26.2 | –0.5 | ... | ... | ... |
42.2 | 2009 02 10 | ... | ... | ... | 2.4 | 28.1 | –0.5 | ... | ... | ... | |
|
|||||||||||
O I | 3.1 | 2009 01 15 | ... | ... | ... | ... | ... | ... | 8.8 | 120.2 | –3.7 |
(8446.36 Å) | 10.4 | 2008 03 19 | –42.1 | 61.3 | –1.5 | ... | ... | ... | 13.5 | 106.1 | –2.1 |
42.2 | 2009 02 10 | ... | ... | ... | ... | ... | ... | 18.8 | 121.2 | –5.5 | |
|
|||||||||||
Ca II | 3.1 | 2009 01 15 | –1.0 | 60.0 | –0.9 | 6.6 | 8.5 | –0.1 | 42.0 | 164.8 | –1.7 |
(8498.02 Å) | 10.4 | 2008 03 19 | –36.3 | 51.1 | –0.6 | –1.3 | 20.9 | –0.5 | 62.8 | 163.6 | –0.6 |
42.2 | 2009 02 10 | –18.4 | 41.4 | –0.6 | 5.9 | 20.2 | –0.7 | 25.7 | 94.1 | –4.1 |
Notes. The listed entries are: line with laboratory wavelength, slit PA, observing date, and for each individual component the velocity at the line peak, the FWHM, and EW. The laboratory wavelengths are taken from the NIST database (http://physics.nist.gov/asd3, Ralchenko et al. 2011). The epochs are listed in the order of increasing slit PA, as in Table 3, for clarity.
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