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red dwarf comparison table
Subject has spectral type is part of has orbital period is an instance of has optical brightness variation has light curve has observational problem has distance has acronym has recovery time has proper motion has amplitude has discoverer has outburst start time has radial velocity is a kind of has peak brightness has name designated with has observable variation time scale has synonym has definition has discovery date has number of star
Barnard's starM5 VOphiuchus25 yearsbinary star   1.83 pc  10.25 arcseconds per year Edward Emerson Barnard 100 km/sec    main sequence starA faint binary star with the second largest proper motion known. Long-term observations of its light curve suggest a possible third component with a mass about 1.2 that of Jupiter, although this observation has been challenged.19162
flare starM   0.2 magnitudes or greater some difficulty in distinguishing between various kinds CV      red dwarf 
  1. R, S, T, U, V, W, X, Y, or Z and the genitive of the latin constellation name
  2. 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
  3. 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
  4. V 335, V 336, etc., when the double letter designations are exhausted
within a period of decadesUV Ceti starStars undergoing erratic jumps in brightness (up to a few magnitudes) on time scales of the order of minutes. During the quiescent phase the spectrum is that of an M dwarf with emissions in the CaII and Balmer lines.  

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