Phact

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Double star
α Columbae
position
AladinLite
Observation
dates equinoxJ2000.0 , epoch : J2000.0
Constellation Dove
Right ascension 05 h 39 m 38.94 s
declination -34 ° 04 ′ 26.8 ″
Apparent brightness 2.65 likes
Typing
B − V color index −0.12 
U − B color index −0.46 
R − I index −0.09 
Spectral class B7 IV
Astrometry
Radial velocity (35.0 ± 4.0) km / s
parallax (12.48 ± 0.36)  mas
distance (261 ± 7)  ly
(80.1 ± 2.3)  pc  
Visual absolute brightness M vis −1.87 mag
Proper movement 
Rec. Share: (1.58 ± 0.28)  mas / a
Dec. portion: (−24.82 ± 0.50)  mas / a
Physical Properties
Dimensions 4.5  M
radius R
Luminosity

1000  L

Effective temperature 12 500  K
Other names
and catalog entries
Bayer name α Columbae
Cordoba Survey CD -34 ° 2375
Bright Star Catalog HR 1956 [1]
Henry Draper Catalog HD 37795 [2]
Hipparcos catalog HIP 26634 [3]
SAO catalog SAO 196059 [4]
Tycho catalog TYC 7064-1357-1 [5]
annotation
  1. estimated from apparent brightness and distance

Phakt (also Phact or Phaet , from Arabic الفاخثة, DMG al-Fāḫita  'dove') is the proper name of the star α Columbae (Alpha Columbae) in the constellation Dove . Phakt is a sub-giant of the spectral class B7e and with an apparent magnitude of 2.65 mag the brightest star of the pigeon. Its distance from Earth is approximately 260 light years . Phakt, like most B stars, rotates very quickly (90 times faster than the sun), so that the rotation speed at the equator is more than 180 km / s. This leads to a flattening of the poles and the formation of a low-density gas disk that surrounds Phakt up to about two star radii away. This disk, excited by its central star, emits an emission line spectrum. Such stars are called Be stars (where the “e” stands for emission). Similar stars are Achernar , Alkione, and Gamma Cassiopeiae .

As a double star, Phakt has a companion that is only 12.3 mag bright at a distance of 13.5 ".

Web link

Individual evidence

  1. a b c Hipparcos catalog (ESA 1997)
  2. a b c Bright Star Catalog
  3. Pulkovo radial velocities for 35493 HIP stars
  4. a b c Hipparcos, the New Reduction (van Leeuwen, 2007)