Basic data (System:981)

C1900.0 :17375+6848
C2000.0 :173657092+68452869
Comp. :A
Magn. : 4.80(V)
Spect. :F5V


Identifiers:

Bayer $\omega$ DraBD +68 949GAIADR2 1637717179389828224GAIADR3 1637717179389828224
GJ 4017HD 160922HIP 86201HR 6596


Orbit

ElementValueStd. dev.
Period (d.):5.2798
Periastron time (xJD-2,400,000.0):40052.6
Reference T0/epoch:JD
Eccentricity:0.04
omega primary (deg.):35.
K1 (km/s):35.4
K2 (km/s):44.6
V0 (km/s):-14.4
sigma residuals primary:
sigma residuals secondary:
#RV primary:
#RV secondary:
Grade:5.0
Contributor:DAO
Status:PUB
Bibcode:1976ApJS...30..273A
Derived quantities (on the fly, from the above quantities)
a1sini (km):2.56807e+060
a2sini (km):3.23548e+060
m1sin**3 i (sol.mass):0.1563690
m2sin**3 i (sol.mass):0.1241140

Note

The new elements obtained by Abt and Levy are preferred to the old ones of A.B.
Turner (Lick Obs. Bull., 4, 163, 1907) because the later observers successfully
resolved the secondary spectrum. The agreement between the two sets is good for
K1 and V0. Since e is small the differences in omega are not important. Both
Luyten and Lucy & Sweeney have revised the original computations by Turner and
have adopted circular orbits, but Abt and Levy find a larger value for e than
Turner did. A brief report on UV emission-line variability in the spectrum of
this star was published by R.A. Stern (Bull. Am. Astron. Soc., 15, 665, 1983).
A 13.2m companion at 72.3" is listed in I.D.S.: according to Abt and Levy it
shares a common proper motion with the spectroscopic binary.

Plot

Orbit
Encapsulated PostScript file

T. Merle

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