RA/DEC (2000) 09:27:41.30 DEC +36:58:22.3
VY LMi has been shown to be a RRab star by Henden and Vidal-Sainz (1997). It was formerly designated as a NSV star suspected to be a cepheid. They found the following elements:
Henden and Vidal-Sainz (1997) also have calibrated some stars in VY LMi field: see table below.
Wils et al. (2006) report observations from ROTSE telescope and derive new elements:
Laurent Corp, Etienne Morelle and Alain Bruno have observed VY LMi with the 60cm telescope at Pic du Midi Observatory during 3 nights between 2008 February 12 and 16. through a V filter.
| date | Julian day | Observer/site | number | filter | ||||
|---|---|---|---|---|---|---|---|---|
| of measurements | ||||||||
| 12 February 2008 | 2454508 | Laurent Corp, Etienne Morelle, Alain Bruno /T60, Pic du Midi | 18 | V | ||||
| 13 February 2008 | 2454509 | Laurent Corp, Etienne Morelle, Alain Bruno /T60, Pic du Midi | 43 | V | ||||
| 16 February 2008 | 2454512 | Laurent Corp, Etienne Morelle, Alain Bruno /T60, Pic du Midi | 43 | V |
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Laurent Corp and collaborators have observed one maximum on 2008 February 13 at HJD 2454509.3715 ± 0.0009. The folded light curve shows that the elements from Henden and Vidal-Sainz (1997) are still up to date. Wils et al.'s (2006) elements are not as precise as shown in O-C diagrams below. |
O-C diagram according to elements from Henden and Vidal-Sainz (1997) |
O-C diagram according to elements from Wils et al.'s' (2006) |