NNo GCVS J2000.0 Type Max Min I Min II Epoch Year Period M-m/D Spectrum References Other desig. p.m.(as/yr) Epoch Ident. New type GCVS
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550003 |T Mon *|062513.00 +070508.6 |DCEP | 5.58 | 6.62 | |V |43784.615 | | 27.024649 |27 |F7Iab-K1Iab+A0V |09029 00559| |+0.003 -0.001|2000.0 | |Hip | |T Mon |
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_______________Cross-identifications:_______________
T Mon = BD +07 1273 |
T Mon = BS 02310 |
T Mon = GSC 0145.00875 |
T Mon = HD 044990 |
T Mon = Hip 030541 |
T Mon = IRAS 06225+0706 |
T Mon = SAO 113845 |
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Reference to a chart or photograph:
00559. A.Wroblewski, Urania 26, 339, 1955.
Reference to a study of the star:
09029. L.Szabados, Bud Mitt N77, 1981.
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Remark:
SB (Porb> = 70 yr [09397]). [A/H] = 0.3.
There is a sguare term in the elements given in the
Table: +5.34d*10**(-6)*E**2.
Deviations from the parabola in the O - C, E diagram
have a wave-like trend. If this wave is attributed to
the light-time effect, Porb = 100 years.
The observations are also satisfied by the following
system of linear elements: Max = 2412874.56 + 27.0093d*E
(JD2405200 - 15250) [09398]; Max = 2426004.62 + 27.0180d*E
(JD2415250 - 27150); since JD2427150 -
Max = 2436137.090 + 27.0205d*E [02392].
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