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I will discuss the so-called two-families scenario in which stars having small radii and masses smaller than a critical one are made of hadrons while the most massive stars are strange quark stars. I will present the main phenomenological implications of that scenario and I will also compare it to the so-called twin-stars scenario. In particular, I will present the many predictions of the two-families scenario that will most likely allow the confirmtion or ruling out of that scheme in the next few years.
Gianluca Cavoto, Raffaella Schneider