Image Details
Caption: Figure 6.
Line identifications in the 2025 September COS Spectrum of BZ Cam. This spectrum (in red) has a continuum flux level of about 20% lower than the one analyzed in P. Godon et al. (2017). The error is shown in black. The spectrum has not been dereddened.
© 2026. The Author(s). Published by the American Astronomical Society.