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 Cephei | 21 18 34.7 | A7V | +62 35 08 | Milky Way | | naked eye star | 2.44 | for many centuries | d | 0.22 | | | asterism | | brighter than 5 | | HR 8162 | | V | |
Alpha Circini | 14 42 30.3 | ApSrEuCr: | -64 58 31 | Milky Way | | naked eye star | 3.19 | for many centuries | | 0.24 | | | asterism | | brighter than 5 | | HR 5463 | | | |
Alpha Coronae Autralis | 19 09 28.2 | A2V | -37 54 16 | Milky Way | | naked eye star | 4.11 | for many centuries | d | 0.04 | | | asterism | | brighter than 5 | | HR 7254 | | V | |
Alpha Coronae Borealis | 15 34 41.2 | A0V | +26 42 53 | Milky Way | | naked eye star | 2.23 | for many centuries | d | -0.02 | | | asterism | | brighter than 5 | | HR 5793 | | V | |
Alpha Doradus | 4 33 59.8 | A0IIISi | -55 2 42 | Milky Way | | naked eye star | 3.27 | for many centuries | | -0.10 | | | asterism | | brighter than 5 | | HR 1465 | | III | |
Alpha Lacertae | 22 31 17.4 | A1V | +50 16 57 | Milky Way | | naked eye star | 3.77 | for many centuries | d | 0.01 | | | asterism | | brighter than 5 | | HR 8585 | | V | |
Alpha Ophiuchi | 17 34 56.0 | A5III | +12 33 36 | Milky Way | | naked eye star | 2.08 | for many centuries | | 0.15 | | | asterism | | brighter than 5 | | HR 6556 | | III | |
Alpha Pictoris | 06 48 11.4 | A7IV | -61 56 29 | Milky Way | | naked eye star | 3.27 | for many centuries | | 0.21 | | | asterism | | brighter than 5 | | HR 2550 | | IV | |
Alpha Sextantis | 10 7 56.2 | A0III | -0 22 18 | Milky Way | | naked eye star | 4.49 | for many centuries | | -0.04 | | | asterism | | brighter than 5 | | HR 3981 | | III | |
Altair | 19 50 46.9 | A7 V | +08 52 06 | Milky Way | | naked eye star | 0.77 | for many centuries | d | 0.22 | 4.8 pc | | asterism | | mv = 0.78 | | HR 7557 | A 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 Trianguli | 2 9 32.5 | A5II | +34 59 14 | Milky Way | | naked eye star | 3.00 | for many centuries | | 0.14 | | | asterism | | brighter than 5 | | HR 622 | | II | |
Canum Venaticorum | 12 56 1.6 | A0pSiEuHg | +38 19 6 | Milky Way | | naked eye star | 2.90 | for many centuries | | -0.12 | | | asterism | | brighter than 5 | | HR 4915 | | | |
Delta Capricorni | 21 47 02.3 | Amv | -16 07 38 | Milky Way | | naked eye star | 2.87 | for many centuries | | 0.29 | | | asterism | | brighter than 5 | | HR 8322 | | | |
Epsilon Ursae Majoris | 12 54 1.7 | A0pCr | +55 57 35 | Milky Way | | naked eye star | 1.77 | for many centuries | | -0.02 | | | asterism | | brighter than 5 | | HR 4905 | | | |
Fomalhaut | 22 57 39.0 | A3 V | -29 37 20 | Milky Way | | naked eye star | 1.16 | for many centuries | d | 0.09 | 7 pc | | asterism | | brighter than 5 | | HR 8728 | An 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. | | |
Sirius | 6 45 8.9 | A1Vm | -16 42 58 | Milky Way | 49.9 years | binary star | -1.46 | for many centuries | d | 0.00 | 8.6 light-years | half the stars in the solar neighborhood are members of star systems | asterism | | brighter than 5 | | HR 2491 | The 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. | V | 2 |
Vega | 18 36 56.2 | A0Va | +38 47 01 | Milky Way | | naked eye star | 0.03 | for many centuries | d | 0.00 | 25 light-years | | asterism | | brighter than 5 | | HR 7001 | The 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. | | |