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Title:
The peculiar horizontal branch morphology of the Galactic globular clusters NGC 6388 and NGC 6441: new insights from UV observations
Authors:
Busso, G.; Cassisi, S.; Piotto, G.; Castellani, M.; Romaniello, M.; Catelan, M.; Djorgovski, S. G.; Recio Blanco, A.; Renzini, A.; Rich, M. R.; Sweigart, A. V.; Zoccali, M.
Affiliation:
AA(INAF - Osservatorio Astronomico di Collurania, via M. Maggini, 64100 Teramo, Italy ; Institut für Theoretische Physik und Astrophysik, University of Kiel, Leibnizstrasse 15, 24114 Kiel, Germany ; Dipartimento di Astronomia, Università di Padova, Vicolo dell'Osservatorio 2, 35122 Padova, Italy), AB(INAF - Osservatorio Astronomico di Collurania, via M. Maggini, 64100 Teramo, Italy ), AC(Dipartimento di Astronomia, Università di Padova, Vicolo dell'Osservatorio 2, 35122 Padova, Italy ), AD(INAF - Osservatorio Astronomico di Roma, via di Frascati 33, 00040, Monte Porzio Catone, Roma, Italy ), AE(European Southern Observatory, Karl Schwarzchild Strasse 2, 85748 Garching, Germany ), AF(Pontificia Universidad Católica de Chile, Departamento de Astronomía y Astrofísica, Av. Vicuña Mackenna 4860, 782-0436 Macul, Santiago, Chile ), AG(Astronomy Department, California Institute of Technology, MC 105-24, Pasadena, CA 91125, USA ), AH(Observatoire de la Côte d'Azur, Dpt. Cassiopée, CNRS/UMR6202, BP 4229, 06304 Nice Cedex 4, France ), AI(INAF - Osservatorio Astronomico di Padova, vicolo Osservatorio 5, 35122 Padova, Italy ), AJ(Department of Physics and Astronomy, UCLA, 430 Portola Plaza, Los Angeles CA, 90095-1547, USA ), AK(NASA Goddard Space Flight Center, Code 667, Greenbelt, MD 20771, USA ), AL(Pontificia Universidad Católica de Chile, Departamento de Astronomía y Astrofísica, Av. Vicuña Mackenna 4860, 782-0436 Macul, Santiago, Chile )
Publication:
Astronomy and Astrophysics, Volume 474, Issue 1, October IV 2007, pp.105-119 (A&A Homepage)
Publication Date:
10/2007
Origin:
EDP Sciences
Keywords:
stars: horizontal-branch, ultraviolet: stars, globular clusters: individual: NGC 6388, globular clusters: individual: NGC 6441
DOI:
10.1051/0004-6361:20077806
Bibliographic Code:
2007A&A...474..105B

Abstract

Context: In this paper we present multiband optical and UV Hubble Space Telescope photometry of the two Galactic globular clusters NGC 6388 and NGC 6441.
Aims: We investigate the properties of their anomalous horizontal branches in different photometric planes in order to shed light on the nature of the physical mechanism(s) responsible for the existence of an extended blue tail and of a slope in the horizontal branch, visible in all the color-magnitude diagrams.
Methods: New photometric data have been collected and carefully reduced. Empirical data have been compared with updated stellar models of low-mass, metal-rich, He-burning structures, transformed to the observational plane with appropriate model atmospheres.
Results: We have obtained the first UV color-magnitude diagrams for NGC 6388 and NGC 6441. These diagrams confirm previous results, obtained in optical bands, about the presence of a sizeable stellar population of extremely hot horizontal branch stars. At least in NGC 6388, we find a clear indication that at the hot end of the horizontal branch the distribution of stars forms a hook-like feature, closely resembling those observed in NGC 2808 and Omega Cen. We briefly review the theoretical scenarios that have been suggested for interpreting this observational feature. We also investigate the tilted horizontal branch morphology and provide further evidence that supports early suggestions that this feature cannot be interpreted as an effect of differential reddening. We show that a possible solution of the puzzle is to assume that a small fraction - ranging between 10-20% - of the stellar population in the two clusters is strongly helium-enriched (Y˜ 0.40 in NGC 6388 and Y˜ 0.35 in NGC 6441). The occurrence of a spread in the He abundance between the canonical value (Y˜ 0.26) and the quoted upper limits can significantly help in explaining the “whole” morphology of the horizontal branch and the pulsational properties of the variable stars in the target clusters.
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