Fig. 5: Spectral energy distributions (SEDs) of the P-rich stars.
From: Phosphorus-rich stars with unusual abundances are challenging theoretical predictions
The SEDs (broad band photometry from 2500 to 250,000 Å in red) for 12 P-rich sample (a–l) stars are shown in comparison with the synthesized fluxes (in black) with the derived stellar parameters and chemical abundances of each star. Error bars show the photometric measurement errors such as provided by VOSA.
