We present the results of a deep photometric survey performed with the VLT FORS1 aimed at investigating the complex main-sequence structure of the stellar system ? Centauri. We confirm the presence of a double main sequence and identify its blue component (bMS) over a large field of view up to 26' from the cluster center. We found that bMS stars are significantly more concentrated toward the cluster center than the other ``normal'' MS stars. The bMS morphology and its position in the CMD have been used to constrain the helium overabundance required to explain the observed MS morphology.
Sollima A., Ferraro F. R., Bellazzini M., Origlia L., Straniero O., Pancino E. (2007). Deep FORS1 Observations of the Double Main Sequence of ω Centauri. THE ASTROPHYSICAL JOURNAL, 654, 915-922 [10.1086/509711].
Deep FORS1 Observations of the Double Main Sequence of ω Centauri
SOLLIMA, ANTONIO;FERRARO, FRANCESCO ROSARIO;
2007
Abstract
We present the results of a deep photometric survey performed with the VLT FORS1 aimed at investigating the complex main-sequence structure of the stellar system ? Centauri. We confirm the presence of a double main sequence and identify its blue component (bMS) over a large field of view up to 26' from the cluster center. We found that bMS stars are significantly more concentrated toward the cluster center than the other ``normal'' MS stars. The bMS morphology and its position in the CMD have been used to constrain the helium overabundance required to explain the observed MS morphology.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
