* Astronomy

Delta Cephei is at minimum brightness at 08:00 UT, 16th February, 2012

Delta Cephei is at minimum brightness at 14:30 UT, 5 February, 2012

Maxima of the variable star Delta Cephei at 19.50 UT, 25th January, 2012.

Title: New Evidence Supporting Cluster Membership for the Keystone Calibrator Delta Cephei
Authors: Daniel J. Majaess, David G. Turner, Wolfgang Gieren

New and existing UBVJHKs, spectroscopic, NOMAD, HST, and revised HIP observations are employed to determine properties for delta Cep and its host star cluster. The multi-faceted approach ensured that uncertainties were mitigated (~2%). The following fundamental parameters were inferred for delta Cep: E(B-V)=0.073±0.018, log(t)=7.9±0.1, and d=272±3(se)±5(sd) pc. The cluster exhibits a turnoff near B6 (M*/Ms~5), and the brightest host cluster members are the supergiants zeta Cep (K1.5Ib) and delta Cep. To within the uncertainties, the two stars share common astrometric parameters (pi, mu_ra, mu_dec, RV ~ -17 km/s) and are tied to bluer members via the evolutionary track implied by the cluster's UBVJHKs colour-colour and colour-magnitude diagrams. The cluster's existence is bolstered by the absence of an early-type sequence in colour-magnitude diagrams for comparison fields. NOMAD data provided a means to identify potential cluster members (n~30) and double the existing sample. That number could increase with forthcoming precise proper motions (DASCH) for fainter main-sequence stars associated with classical Cepheids (e.g., delta Cep), which may invariably foster efforts to strengthen the Galactic Cepheid calibration and reduce uncertainties tied to H_0.

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