Volume 535, November 2011
|Number of page(s)||16|
|Section||Galactic structure, stellar clusters and populations|
|Published online||23 November 2011|
A Strömgren view of the multiple populations in globular clusters
INAF – Osservatorio Astronomico di Bologna, via Ranzani 1, 40127 Bologna, Italy
e-mail: email@example.com; firstname.lastname@example.org
2 INAF – Osservatorio Astronomico di Padova, Vicolo dell’Osservatorio 5, 35122 Padova, Italy
e-mail: email@example.com; firstname.lastname@example.org; email@example.com
Received: 3 May 2011
Accepted: 8 September 2011
We discuss a variety of photometric indices assembled from the uvby Strömgren system. Our aim is to examine the pros and cons of the various indices to find the most suitable one(s) for studying the properties of multiple populations in the globular clusters (GCs) discovered by spectroscopy. We explore in particular the capabilities of indices like m1 and cy at different metallicities. We define a new index δ4 = (u − v) − (b − y) to separate first and second stellar generations in GCs of any metal abundance, since it keeps the sensitivity to multiple stellar populations over the full metallicity range and at the same time minimizes the sensitivity to photometric errors. We detect clear differences in the red giant branches of the GCs examined, such as skewness or bi/multimodality in color distribution. We connect the photometric information with the spectroscopic results on the O and Na abundances we obtained in our survey of GCs. Finally, we compute the effects of different chemical composition on the Strömgren filters and indices using synthetic spectra.
Key words: stars: abundances / stars: atmospheres / stars: Population II / globular clusters: general
© ESO, 2011
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