Table 4
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Results of Gaussian fitting to observed spectra. Shown are the observation dates, including time since outburst, and individual components FWHM and radial velocity displacement in km s−1. Components 1 and 4 relate to the polar blobs, component 2 to the equatorial ring and component 3 to the prolate structure described in Section 6.2.

DayComponent 1Component 2Component 3Component 4
FWHMRadialFWHMRadialFWHMRadialFWHMRadial
+2.342128−3422982−1773791−17722583251
+3.342152−3466844−2203717−22021723116
+5.312310−3425528−2253083−22523193066
+8.332283−3361333−2513598−25123142994
DayComponent 1Component 2Component 3Component 4
FWHMRadialFWHMRadialFWHMRadialFWHMRadial
+2.342128−3422982−1773791−17722583251
+3.342152−3466844−2203717−22021723116
+5.312310−3425528−2253083−22523193066
+8.332283−3361333−2513598−25123142994
Table 4
Open in new tab

Results of Gaussian fitting to observed spectra. Shown are the observation dates, including time since outburst, and individual components FWHM and radial velocity displacement in km s−1. Components 1 and 4 relate to the polar blobs, component 2 to the equatorial ring and component 3 to the prolate structure described in Section 6.2.

DayComponent 1Component 2Component 3Component 4
FWHMRadialFWHMRadialFWHMRadialFWHMRadial
+2.342128−3422982−1773791−17722583251
+3.342152−3466844−2203717−22021723116
+5.312310−3425528−2253083−22523193066
+8.332283−3361333−2513598−25123142994
DayComponent 1Component 2Component 3Component 4
FWHMRadialFWHMRadialFWHMRadialFWHMRadial
+2.342128−3422982−1773791−17722583251
+3.342152−3466844−2203717−22021723116
+5.312310−3425528−2253083−22523193066
+8.332283−3361333−2513598−25123142994
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