V394 Aurigae

From Wikipedia, the free encyclopedia
Jump to navigation Jump to search

Template:Short description

V394 Aurigae
Template:Location mark
Location of V394 Aurigae (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Auriga
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) 6.01 - 6.11[2]
Characteristics
Evolutionary stage AGB[3]
Spectral type M3II[4]
U−B Template:Engvar 1.94
B−V Template:Engvar 1.73
Variable type Semi-regular[2]
Astrometry
Radial velocity (Rv)Script error: No such module "val".[5] km/s
Proper motion (μ) RA: 11.503[1] mas/yr
Dec.: −5.126[1] mas/yr
Parallax (π)3.7146±0.0756 mas[1]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Details
Radius85[6] Template:Solar radius
Luminosity985[1] Template:Solar luminosity
Surface gravity (log g)0.78[7] cgs
Temperature3,639[6] K
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
DO 11899, HIC 28930, PPM Star Catalogue 95388, STT 129, GC 7725, HIP 28930, SAO 77958, ADS 4673, GCRV 3829, HR 2146, AG+29° 663, IDS 06000+2931, TYC 1876-1774-1, BD+29° 1112, IRAS 06031+2931, UBV M 11751, CCDM J06064+2931, GSC 01876-01774, IRC +30137, YZ 29 2943, CSI+29 1112 1, HD 41429, 2MASS J06062243+2930445.
Database references
SIMBADdata

Script error: No such module "Check for unknown parameters".

File:V394AurLightCurve.png
A light curve for V394 Aurigae, plotted from Hipparcos data[8]

V394 Aurigae is a semi-regular variable star in the constellation Auriga. Its brightness varies between magnitudes 6.01 and 6.11,[2] so it is faintly visible to the naked eye under ideal observing conditions. Located around 730 light-years distant, V394 Aurigae shines with a luminosity approximately 985 times that of the Sun[1] and has a surface temperature of Script error: No such module "val"..[6]

In 1991, Leroy F. Snyder discovered that the star, then called HR 2146, is a variable star.[9] It was given its variable star designation, V394 Aurigae, in 1993.[10] Koen and Eyer found that the star's brightness, as seen by Hipparcos, varies with a period of 3.9 days.[11]

It is a double star: the secondary, designated V394 Aurigae B, is an eleventh-magnitude F7V star[12] with a separation of 10 arcseconds.[13]

References

<templatestyles src="Reflist/styles.css" />

  1. ↑ a b c d e f g Template:Cite DR2
  2. ↑ a b c Script error: No such module "citation/CS1".
  3. ↑ Script error: No such module "Citation/CS1".
  4. ↑ Script error: No such module "Citation/CS1".
  5. ↑ Script error: No such module "Citation/CS1".
  6. ↑ a b c Script error: No such module "Citation/CS1".
  7. ↑ Script error: No such module "Citation/CS1".
  8. ↑ Script error: No such module "citation/CS1".
  9. ↑ Script error: No such module "Citation/CS1".
  10. ↑ Script error: No such module "Citation/CS1".
  11. ↑ Script error: No such module "Citation/CS1".
  12. ↑ Script error: No such module "Citation/CS1".
  13. ↑ Script error: No such module "Citation/CS1". Vizier catalog entry

Script error: No such module "Check for unknown parameters".

Template:Stars of Auriga

Retrieved from "http://debianws.lexgopc.com/wiki143/index.php?title=V394_Aurigae&oldid=7273491"