Persistent nuclear burning in Nova Sgr 2016 N.4 (=V5856 Sgr = ASASSN-16ma) six years past its outburst

Open Access

Fig. 6.

Region around NaI 5890 and KI 7699 from averaged CHIRON spectra listed in Table 2. The interstellar components at −21.8 and +4.3 km s⁻¹ velocity are indicated, as is their decovolution (discussed in Sect. 4.3). The broad absorption labeled “wind” is variable from spectrum to spectrum.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.