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URL: http://sv.wikipedia.org/wiki/W_Bootis

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W Bootis

Från Wikipedia
W Bootis
Observationsdata
Epok: J2000.0
StjärnbildBjörnvaktaren
Rektascension14t 43m 25,36s
Deklination+26° 31′ 40,27″[1]
Skenbar magnitud ()+4,62 (maximum), 4,93 (minimum) [2]
Stjärntyp
SpektraltypM4.5e[1]
B–V1,672±0,006[3]
VariabeltypHalvregelbunden variabel (SRB)[2]
Astrometri
Radialhastighet ()5,60 ± 0,49 km/s
Egenrörelse (µ)RA: -13,57 ± 0,29 mas/år
Dek.: -16,08 ± 0,27 mas/år
Parallax ()4,63±0,28 mas
Andra beteckningar
34 Bootis, GSC 02019-01252, N30 3327, TYC 2019-1252-1, HD 129712, PLX 3331, UBV 12835, AG+26 1447, HIC 71995, PLX 3331.00, UBV M 20330, BD+27 2413, HIP 71995, PMC 90-93 971, YZ 26 6950, DO 15058, HR 5490, PPM 103535, HFE83 1047, FK5 1383, IRAS 14412+2644, RAFGL 1724, AAVSO 1439+26, GC 19831, IRC +30263, SAO 83488, GCRV 8555, JP11 2532, SKY# 26751, GEN# +1.00129712, 2MASS J14432536+2631402, SRS 31383[1]

W Bootis är en halvregelbunden variabel av SRB-typ[2] i stjärnbilden Björnvaktaren.

Stjärnan varierar mellan fotografisk magnitud +4,62 och 4,93 med en period av 25,51 dygn.[2]

  1. ^ [a b c] ”Basic data: V* 34 Boo – Long-period variable star” (på engelska). Centre de Données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=W+Boo&submit=SIMBAD+search. Läst 28 april 2016. 
  2. ^ [a b c d] ”W Boo” (på engelska). The International Variable Star Index. AAVSO – American Association of Variable Star Observers. http://www.aavso.org/vsx/index.php?view=detail.top&oid=4309. Läst 28 april 2016. 
  3. ^ van Leeuwen (2007). ”Hipparcos, the New Reduction” (på engelska). http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=I/311/hip2&HIP=71995. Läst 28 april 2017. 
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