| YY Orionis star | has spectra peculiarity inverse P Cyg type emission profiles in the Ca II HK lines |   | 
| has definition Very young, late-type, low-mass stars in the gravitationally contracting stage in which the star is still accreting matter from the protostellar cloud. |   | 
| is a kind of T Tauri star |   | 
| T Tauri star | has synonym nebular variable |   | 
| late star | has spectral type cooler than G2 |   | 
| emission line star | has emission line |   | 
| star | has star surface temperature |   | 
| has V magnitude |   | 
| has B magnitude |   | 
| has U magnitude |   | 
| has position on celestial sphere from the point of view of Earth |   | 
| has parallax from the point of view of Earth's orbit |   | 
| has proper motion |   | 
| has radiation at surface which is diffused out from the hotter core |   | 
| has energy source gravitational contraction and or fusion |   | 
| has energy production which takes place primarily within the core |   | 
| has surface density which depends on luminosity class |   | 
| has surface temperature greater than 1000 Kelvin |   | 
| has apparent magnitude |   | 
| has absolute magnitude |   | 
| has age |   | 
| has catalog star catalog |   | 
| has material hydrogen, helium |   | 
| has velocity determined from proper motion and radial velocity |   | 
| has mass greater than 0.08 the sun's mass |   | 
| variable | has name designated with - R, S, T, U, V, W, X, Y, or Z and the genitive of the latin constellation name
 - RR, RS, RT, RU, RV, RW, RX, RY, or RZ and the genitive of the latin constellation name when the single letter designations are exhausted
 - AA...AZ, BB...BZ, etc. (omitting J), which ends with QQ...QZ and the genitive of the latin constellation namewhen the RR...RZ designations are exhausted
 - V 335, V 336, etc., when the double letter designations are exhausted
 
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| has observational problem some difficulty in distinguishing between various kinds |   | 
| has observable variation time scale within a period of decades |   | 
| has light curve |   | 
| has optical brightness variation 0.2 magnitudes or greater |   | 
| has amplitude |   | 
| celestial body | has spectra |   | 
| physical object | has location or center of gravity |   | 
| has angular momentum |   | 
| has momentum |   | 
| has temperature |   | 
| has volume |   | 
| has extent |   |