The term
iron star was applied to a star called "XX Oph" or "Merrill's Iron Star" with a complex, highly variable spectrum with a forest of Fe II emission lines. First discovered in 1908 by
Williamina Fleming, it was studied over 30 years by
Paul W. Merrill. The star is believed to be a non-eclipsing binary star. A second binary star, AS 325, has a similar spectrum and complex spectral variability and has been characterized as the second iron star. ==Blue supergiant==