Preliminary results from the STEPHI2009 campaign on the open cluster NGC 1817

Details Preliminary results from the STEPHI2009 campaign on the open cluster NGC 1817 Preliminary results from the STEPHI2009 campaign on the open cluster NGC 1817

2010-04-14

arxiv.org/abs/1004.2348v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

4 pages, proceedings from HELAS IV meeting 2010, Lanzarote

Scientific paper

We present preliminary observational results of the multi-site STEPHI campaign on the cluster NGC 1817. The three observatories involved are San Pedro Martir (Mexico), Xing Long (China) and the Observatorio del Teide (Spain) - giving an ideal combination to maximise the duty cycle. The cluster has 12 known delta Scuti stars and at least two detached eclipsing binary systems. This combination of characteristics is ideal for extracting information about global parameters of the targets, which will in turn impose strict constraints on the stellar models. From an initial comparison with stellar models using the known fundamental parameters, and just the observed pulsation frequencies and measured effective temperatures, it appears that a lower value of initial helium mass fraction will most likely explain the observations of these stars.

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