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A star comparison table
Subject has right ascension has spectral type has declination is part of has orbital period is an instance of has V magnitude has been observ has symbol has B-V magnitude has distance has abundance is usually part of is a kind of has apparent magnitude has emission line has synonym has definition has luminosity class has number of star
Ae star             A star one or several Balmer lines A-type star with emission in one or several Balmer lines.  
Alpha Cephei21 18 34.7A7V+62 35 08Milky Way naked eye star2.44for many centuriesd0.22  asterism brighter than 5 HR 8162 V 
Alpha Circini14 42 30.3ApSrEuCr:-64 58 31Milky Way naked eye star3.19for many centuries 0.24  asterism brighter than 5 HR 5463   
Alpha Coronae Autralis19 09 28.2A2V-37 54 16Milky Way naked eye star4.11for many centuriesd0.04  asterism brighter than 5 HR 7254 V 
Alpha Coronae Borealis15 34 41.2A0V+26 42 53Milky Way naked eye star2.23for many centuriesd-0.02  asterism brighter than 5 HR 5793 V 
Alpha Doradus4 33 59.8A0IIISi-55 2 42Milky Way naked eye star3.27for many centuries -0.10  asterism brighter than 5 HR 1465 III 
Alpha Lacertae22 31 17.4A1V+50 16 57Milky Way naked eye star3.77for many centuriesd0.01  asterism brighter than 5 HR 8585 V 
Alpha Ophiuchi17 34 56.0A5III+12 33 36Milky Way naked eye star2.08for many centuries 0.15  asterism brighter than 5 HR 6556 III 
Alpha Pictoris06 48 11.4A7IV-61 56 29Milky Way naked eye star3.27for many centuries 0.21  asterism brighter than 5 HR 2550 IV 
Alpha Sextantis10 7 56.2A0III-0 22 18Milky Way naked eye star4.49for many centuries -0.04  asterism brighter than 5 HR 3981 III 
Altair19 50 46.9A7 V+08 52 06Milky Way naked eye star0.77for many centuriesd0.224.8 pc asterism mv = 0.78 HR 7557A bright A7 V star.V 
Am star O, B, A, and early F           A star   A-type or F-type object to which no unique spectral type can be assigned. Usually the classifier provides a classification according to the hydrogen, metallic and calcium lines. Also call metallic-line stars.  
Ap star O, B, A, and early F           A star   Peculiar A-type stars ("magnetic" A stars) that show abnormally strong lines, sometimes of varying intensity, of certain ionized metals. Recent evidence indicates that all Ap stars are slow rotators compared with normal A stars.  
Beta Trianguli2 9 32.5A5II+34 59 14Milky Way naked eye star3.00for many centuries 0.14  asterism brighter than 5 HR 622 II 
Canum Venaticorum12 56 1.6A0pSiEuHg+38 19 6Milky Way naked eye star2.90for many centuries -0.12  asterism brighter than 5 HR 4915   
Delta Capricorni21 47 02.3Amv-16 07 38Milky Way naked eye star2.87for many centuries 0.29  asterism brighter than 5 HR 8322   
Epsilon Ursae Majoris12 54 1.7A0pCr+55 57 35Milky Way naked eye star1.77for many centuries -0.02  asterism brighter than 5 HR 4905   
Fomalhaut22 57 39.0A3 V-29 37 20Milky Way naked eye star1.16for many centuriesd0.097 pc asterism brighter than 5 HR 8728An A star. The brightest star in the constellation Piscis Austrinus.V 
Magnetic star O, B, A, and early F           A star   Star (usually of spectral type A) with strong integrated magnetic fields ranging up to 30000 gauss.  
Sirius6 45 8.9A1Vm-16 42 58Milky Way49.9 yearsbinary star-1.46for many centuriesd0.008.6 light-yearshalf the stars in the solar neighborhood are members of star systemsasterism brighter than 5 HR 2491The brightest star in the sky. Its companion (Sirius B) is a white dwarf of about 0.96 Msun but only about 0.03 Rsun, the nearest white dwarf to Earth.V2
Vega18 36 56.2A0Va+38 47 01Milky Way naked eye star0.03for many centuriesd0.0025 light-years asterism brighter than 5 HR 7001The fifth brightest star in the night sky.V 
white giant             A star   A giant star of spectral type A. Some RR Lyrae stars are white giants.III 
white supergiant O, B, A, and early F           A star   A supergiant star with a spectral type of A. White supergiants are rare; the nearest is Deneb, which lies 1500 light-years away.  

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