Hostname: page-component-cd9895bd7-8ctnn Total loading time: 0 Render date: 2024-12-26T13:00:33.434Z Has data issue: false hasContentIssue false

Integrated spectral properties of star clusters in the Magellanic Clouds

Published online by Cambridge University Press:  01 July 2008

Andrea V. Ahumada
Affiliation:
European Southern Observatory - ESO, Chile, email: [email protected] Observatorio Astronómico, Universidad Nacional de Córdoba, Argentina Consejo Nacional de Investigaciones Científicas y Técnicas, CONICET, Argentina
M. L. Talavera
Affiliation:
Observatorio Astronómico Centroamericano de Suyapa, UNAH, Honduras
J. J. Clariá
Affiliation:
Observatorio Astronómico, Universidad Nacional de Córdoba, Argentina Consejo Nacional de Investigaciones Científicas y Técnicas, CONICET, Argentina
J. F. C. Santos Jr.
Affiliation:
Departamento de Física, ICEx, UFMG, Belo Horizonte, Brazil
E. Bica
Affiliation:
Departamento de Astronomia, UFRGS, Porto Alegre, Brazil
M. C. Parisi
Affiliation:
Observatorio Astronómico, Universidad Nacional de Córdoba, Argentina Consejo Nacional de Investigaciones Científicas y Técnicas, CONICET, Argentina
M. C. Torres
Affiliation:
Observatorio Astronómico, Universidad Nacional de Córdoba, Argentina
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We present flux-calibrated integrated spectra in the optical spectral range of concentrated star clusters in the Large and Small Magellanic Clouds (LMC-SMC), approximately half of which constitute unstudied objects. We have mainly estimated ages and foreground interstellar reddening values from the comparison of the line strengths and continuum distribution of the cluster spectra with those of template spectra with known parameters. Also reddening values were estimated by interpolation between the extinction maps of Burstein & Heiles (1982) (BH). A good agreement between ages and reddenings derived through the different procedures was found. The ages of the 27 LMC star clusters range from 5 to 125 Myr, while those of the 13 SMC vary from 4 to 350 Myr.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2009

References

Bica, E. 1988, A&A, 195, 76Google Scholar
Bica, E. & Alloin, D. 1986a, A&A, 162, 21Google Scholar
Bica, E. & Alloin, D. 1986b, A&AS, 66, 171Google Scholar
Bruck, M. T. 1976, Occasional Reports R. Obs., 1, 1Google Scholar
Burstein, D. & Heiles, C. 1982, AJ, 87, 1165 (BH)Google Scholar
Hodge, P. W. & Wright, F. W. 1974, AJ, 79, 858CrossRefGoogle Scholar
Hodge, P. W. & Sexton, J. A. 1966, AJ, 71, 363CrossRefGoogle Scholar
Kontizas, M., Morgan, D. H., Hatzidimitriou, D., & Kontizas, E. 1990, A&AS, 84, 527Google Scholar
Kron, G. E. 1956, PASP, 68, 125Google Scholar
Lauberts, A. 1982, The ESO/Uppsala Survey of the ESO (B) Atlas, (European Southern Observatory)Google Scholar
Lindsay, E. M. 1958, MNRAS, 118, 172Google Scholar
Lyngå, G. & Westerlund, B. E. 1963, MNRAS, 127, 31Google Scholar
Piatti, A. E., Bica, E., Clariá, J. J., Santos, J. F. C. Jr., & Ahumada, A. V. 2002, MNRAS, 335, 233Google Scholar
Pietrzyński, G., Udalski, A., Kubiak, M., Szymański, M., Woźniak, P., & Żebruń, K. 1998, AcA, 48, 175Google Scholar
Pietrzyński, G., Udalski, A., Kubiak, M., Szymański, M., Woźniak, P., & Żebruń, K. 1999, AcA, 49, 521Google Scholar
Santos, J. F. C. Jr., Bica, E., Clariá, J. J., Piatti, A. E., Girardi, L. A., & Dottori, H. 1995, MNRAS, 276, 1155Google Scholar
Santos, J. F. C. Jr., & Piatti, A. E. 2004, A&A, 428, 79Google Scholar
Searle, L., Wilkinson, A., & Bagnuolo, W. G. 1980, ApJ, 239, 803Google Scholar
Seaton, M. J. 1979, MNRAS, 187, 73pGoogle Scholar
Shapley, H. & Lindsay, E. M. 1963, Irish Astron. J., 6, 74Google Scholar
Talavera, M. L., Ahumada, A. V., Clariá, J. J., Parisi, M. C., Santos, J. F. C. Jr., & Bica, E. 2006, BAAA, 49, 311Google Scholar
Westerlund, B. E. & Glaspey, J. 1971, A&A, 10, 1Google Scholar