Basic data (System:1795)

C1900.0 :
C2000.0 :18122216-1140071
Comp. :A
Magn. : 5.10(K)
Spect. :M3.5III


Identifiers:

GAIADR2 4156835340974302464GAIADR3 4156835340974302464GCVS V343 SerMisc AS 289
Misc Hen 3-1627Misc SS73 143


Orbit

ElementValueStd. dev.
Period (d.):450.52.2
Periastron time (xJD-2,400,000.0):50674.719.6
Reference T0/epoch:JD
Eccentricity:0.1350.046
omega primary (deg.):218.616.2
K1 (km/s):2.660.12
K2 (km/s):
V0 (km/s):-5.6520.083
sigma residuals primary:
sigma residuals secondary:
#RV primary:21
#RV secondary:
Grade:5
Contributor:FKL
Status:PUB
Bibcode:2001AJ....121.2219F
Derived quantities (on the fly, from the above quantities)
a1sini (km):1.63274e+07750000
f(m) (sol.mass):0.0008578660.00012

Note

The system is a symbiotic binary consisting of an M giant and a probable hot
compact companion.  Radial velocities were measured from absorption lines in
the infrared.

The criteria of Lucy and Sweeney (1971, AJ, 76, 644) indicate that the
eccentric-orbit solution is to be preferred, but the results are relatively
close to the dividing lines of both tests.

asini = 16330000 +/- 740000 km
f(m) = 0.00086 +/- 0.00012 solar masses

Radial velocities used in this orbit

xJDRad.Vel.O-C or errorWeightComponentOffsetComment
-2,400,000.0(km/s)(km/s)(km/s)
49802.984-6.60.31.0a
49874.917-4.5-0.51.0a
49923.736-3.30.01.0a
49998.588-4.1-0.31.0a
50161.950-8.20.21.0a
50253.711-6.70.21.0a
50254.793-7.0-0.21.0a
50319.755-3.90.31.0a
50386.578-3.00.31.0a
50567.876-7.00.21.0a
50628.809-8.8-0.21.0a
50752.587-5.1-0.31.0a
50934.820-4.30.31.0a
50983.798-6.1-0.11.0a
51052.645-8.6-0.51.0a
51294.962-3.10.21.0a
51363.703-4.10.01.0a
51415.704-5.8-0.31.0a
51480.590-7.00.51.0a
51647.910-4.90.11.0a
51831.609-4.7-0.21.0a


Plot

Orbit
Encapsulated PostScript file

T. Merle

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