Hello all,
Here is my new update for the monitoring of the outburst of RS Oph with two new spectra obtained with my Alpy 600.
The first one, the 14th of August at 21 h 06 TU (resolution of 521, JJ = 2459441.3793) and an acquisition time of 15 min s (60 x 15 s) :

- RS Oph on August 14th, 2021
- _rsoph_20210814_879_Christophe Boussin_3700_7565.png (66.63 KiB) Viewed 9629 times
The second one, the 15th of August at 21 h 15 TU (resolution of 535, JJ = 2459442.3853) and an acquisition time of 7 min s (14 x 30 s) :

- RS Oph on August 15th, 2021
- _rsoph_20210815_885_Christophe Boussin_3700_7565.png (67.19 KiB) Viewed 9629 times
The relative intensities of the Balmer lines have increased significantly as well as those of HeI :

- RS Oph on August 13th, 14th and 15th 2021
Overall, the relative intensities of the FeII lines seem to have changed very little.
The larger increase in the relative intensity of some FeII lines seems to be due to the presence of HeI lines blended with them (e.g. at 4923 and 5018 A) :

- RS Oph on August 13th, 14th and 15th 2021 (identification of some lines from PlotSpectra)
Clear skies to all !!
Christophe BOUSSIN
CBO (Newton 200 F/5 / Alpy600 / Atik 314L+ / Atik Titan + Mewlon 180 F/12 / LHIRES III 2400 / Atik 460EX / Atik 314 L+) @ ARAS database