Subject |
has right ascension |
has spectral type |
has declination |
is part of |
has surface temperature |
has orbital period |
is an instance of |
has heliocentric radial velocity |
has V magnitude |
has been observ |
has symbol |
has B-V magnitude |
has distance |
has prototype |
has abundance |
is usually part of |
has proper motion |
has discoverer |
has radial velocity |
is a kind of |
has apparent magnitude |
has emission line |
has synonym |
has definition |
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has luminosity class |
has discover |
has number of star |
Alpha Vulpeculae | 19 28 42.2 | M0III | +24 39 54 | Milky Way | greater than 1000 Kelvin | | naked eye star | | 4.44 | for many centuries | | 1.50 | | | | asterism | | | | | brighter than 5 | | HR 7405 | | | III | | |
Barnard's star | | M5 V | | Ophiuchus | greater than 1000 Kelvin | 25 years | binary star | | | | d | | 1.83 pc | | 70 percent of all stars | | 10.25 arcseconds per year | Edward Emerson Barnard | 100 km/sec | | | | main sequence star | A 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. | 1916 | V | | 2 |
dMe star | | dKe star, dMe star | | | greater than 1000 Kelvin | | | | | | d | | | UV Ceti | | | | | | M star | | hydrogen | main sequence star | M dwarf with hydrogen emission lines. | | V | | |
Gamma Sagittae | 19 58 45.3 | M0III | +19 29 32 | Milky Way | greater than 1000 Kelvin | | naked eye star | | 3.47 | for many centuries | | 1.57 | | | | asterism | | | | | brighter than 5 | | HR 7635 | | | III | | |
Kapteyn's star | | M0 | | | greater than 1000 Kelvin | | subdwarf | | | | sd | | 13 light-years | | | | | | +242 km s-1 | | | | CD -45 1841 | A nearby high-velocity M0 subdwarf that is both the nearest halo star to the Sun and the nearest star that orbits the Galaxy backward. | 1897 | VI | Jacobus Kapteyn | |
Kruger 60 AB | | cooler than G2 | | | greater than 1000 Kelvin | P = 44.5 years | binary star | | | | d | | 3.93 pc | | half the stars in the solar neighborhood are members of star systems | | | | | | 12 | | main sequence star | A faint dM binary in the Solar neighborhood. It may be a subluminous star. | | V | | 2 |
Me star | | | | | greater than 1000 Kelvin | | | | | | | | | | | | | | | M star | | | | Star of spectral type M with emission lines in their spectra. | | | | |
MS star | | cooler than G2 | | | greater than 1000 Kelvin | | | | | | | | | | | | | | | M star | | | | M-type stars with ZrO bands. | | | | |
NML Cygnus | | M6 III | | Cygnus | 700 K | | giant | -43 km s-1 | | | | | 200 pc | | | | | Neugebauer, Martz, and Leighton | | | | | IRC+40448 | An infrared star. Its surface temperature is about the same as the surface temperature of Venus. It is a strong OH emitter, and CO has been identified in its spectrum. | | III | | |
red giant | | | | | greater than 1000 Kelvin | | | | | | | | | | | | | | | M star | | | | A late-type (K or M) high-luminosity (brighter than Mv = 0) star that occupies the upper right portion of the H-R diagram. Red giants are post-main-sequence stars that have exhausted the nuclear fuel in their cores. The red-giant phase corresponds to the establishment of a deep convective envelope. Red giants in a globular cluster are about 3 times more luminous than RR Lyrae stars in the same cluster. | | III | | |