Alright, one of the most interesting questions about blue ellipticals is whether the star formation in them is basically confined to the center of the galaxy, or whether it is extended. When I measure the star formation rate using indicators in the SDSS spectra, I can only probe the "central" star formation rate, as the spectra only cover the center of the galaxy. I've used two other star formation rate indicators (ultraviolet and infrared light) for the *whole* galaxy and found a much higher star formation rate. This means that the star formation in blue ellipticals must be extended across much of the galaxy.