Basic data (System:662)
C1900.0 | : | 11079-6033
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C2000.0 | : | 111204506-61054293
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Comp. | :
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Magn. | : | 8.72
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Spect. | : | O7.5 ; O8.5
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Identifiers:
CD -60 3419 | CPD -60 2638 | GAIADR2 5337239658437912960 | GAIADR3 5337239658437912960
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GCVS EM Car | HD 97484 | TYC 8959-569-1
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Orbit
Element | | Value | Std. dev.
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Period (d.) | : | 3.4143 |
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Primary minimum (xJD-2,400,000.0) | : | 46093.986 |
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Reference T0/epoch | : | JD
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Eccentricity | : | 0.02 |
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omega primary (deg.) | : | |
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K1 (km/s) | : | 236. |
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K2 (km/s) | : | 263. |
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V0 (km/s) | : | -18. |
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sigma residuals primary | : |
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sigma residuals secondary | : |
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#RV primary | : |
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#RV secondary | : |
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Grade | : | 2.0
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Contributor | : | DAO
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Status | : | PUB
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Bibcode | : | 1986PASP...98..788S
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Derived quantities (on the fly, from the above quantities) |
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a1sini (km) | : | 1.1078e+07 | 0
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a2sini (km) | : | 1.23454e+07 | 0
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m1sin**3 i (sol.mass) | : | 23.2413 | 0
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m2sin**3 i (sol.mass) | : | 20.8553 | 0
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Note
The epoch is the time of primary minimum. The elements given are derived from
measures of the helium lines and the small eccentricity probably should be
neglected, especially since no value is given for omega. Measures of the
hydrogen lines lead to the derivation of a more eccentric orbit and lower
semi-amplitudes. No photoelectric light-curve is available; the system was
shown to be eclipsing from photographic observations (S. Gaposchkin, Ann. Harv.
Coll. Obs., 113, No. 2, 1953).
Plot
Encapsulated PostScript file
T. Merle