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Title:
Spectroscopy of horizontal branch stars in NGC 6752. Anomalous results on atmospheric parameters and masses
Authors:
Moni Bidin, C.; Moehler, S.; Piotto, G.; Momany, Y.; Recio-Blanco, A.
Affiliation:
AA(Dipartimento di Astronomia, Università di Padova, Vicolo dell'osservatorio 3, 35122 Padova, Italy ; Departamento de Astronomía, Universidad de Chile, Casilla 36-D, Santiago, Chile ), AB(European Southern Observatory, Karl-Schwarzschild-Str. 2, 85748 Garching, Germany), AC(Dipartimento di Astronomia, Università di Padova, Vicolo dell'osservatorio 3, 35122 Padova, Italy), AD(INAF - Osservatorio Astronomico di Padova, Vicolo dell'osservatorio 2, 35122 Padova, Italy), AE(Observatoire de la Côte d'Azur, Dpt. Cassiopée, CNRS UMR 6202, BP 4229, 06304 Nice Cedex 04, France)
Publication:
Astronomy and Astrophysics, Volume 474, Issue 2, November I 2007, pp.505-514 (A&A Homepage)
Publication Date:
11/2007
Origin:
EDP Sciences
Keywords:
stars: horizontal-branch, stars: fundamental parameters, globular clusters: individual: NGC 6752
DOI:
10.1051/0004-6361:20078184
Bibliographic Code:
2007A&A...474..505M

Abstract

Context: The determination of fundamental parameters for horizontal branch stars in Galactic globular clusters frequently gives puzzling results, pointing to the lack of our understanding of their atmospheric structure and the inadequate approximations by the models.
Aims: We wanted to measure effective temperatures, surface gravities, helium abundances, and masses for hot horizontal branch stars in NGC 6752 in order to compare the results with evolutionary predictions.
Methods: We used the ESO VLT-FORS2 facility to collect low-resolution spectra of 51 targets distributed along the horizontal branch. We determined atmospheric parameters, by comparison with theoretical models through standard fitting routines, and masses by basic equations.
Results: Results generally agree with previous works, although not always with the theoretical expectations for cooler stars (T_eff≤ 15 000 K). The calculated color excess is systematically lower than the literature values, pointing towards a possible underestimation of effective temperatures. Moreover, we find two groups of stars at T_eff˜14 000 K and at T_eff˜27 000 K that present anomalies with respect to the general trend and expectations. We suppose that the three peculiar bright stars at T_eff˜14 000 K are probably affected by an enhanced stellar wind. For the eight extreme horizontal branch stars at T_eff˜27 000 K that show unusually high masses, we find no plausible explanation.
Conclusions: While most of our results agree well with the predictions of standard horizontal branch evolution, we still have problems with the low masses we derive in certain temperature ranges. We believe that Kurucz ATLAS9 LTE model atmospheres with solar-scaled abundances are probably inadequate for these temperature ranges. Concerning the group of anomalous stars at T_eff˜27 000 K, a Kolmogorov-Smirnov test indicates that there is only an 8.4% probability that these stars are randomly drawn from the general distribution in the color-magnitude diagram. This is not conclusive but indicates that these stars could be both (and independently) spectroscopically and photometrically peculiar with respect to the general extreme horizontal branch population.

Based on observations with the ESO Very Large Telescope at Paranal Observatory, Chile (proposal ID 69.D-0682).

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