YY Orionis starAn extremely young star, preceding even the T Tauri stage. YY Orionis stars are very young, late-type, low-mass stars, still contracting gravitationally and accreting matter from the protostellar cloud. They show inverse P Cygni profiles corresponding to an infall of material at 300–400 km/s directly onto the star. Related entry• variable starsRelated category• TYPES OF STARAlso on this site: Encyclopedia of Alternative Energy & Sustainable Living Encyclopedia of History |