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The IACOB spectroscopic database of galactic OB stars

Published online by Cambridge University Press:  12 July 2011

Sergio Simón-Díaz ,
Norberto Castro ,
Miriam Garcia  and
Artemio Herrero
Sergio Simón-Díaz
Affiliation:
Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain Departamento de Astrofísica, Universidad de La Laguna, E-38205 La Laguna, Tenerife, Spain
Norberto Castro
Affiliation:
Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain Departamento de Astrofísica, Universidad de La Laguna, E-38205 La Laguna, Tenerife, Spain
Miriam Garcia
Affiliation:
Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain Departamento de Astrofísica, Universidad de La Laguna, E-38205 La Laguna, Tenerife, Spain
Artemio Herrero
Affiliation:
Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain Departamento de Astrofísica, Universidad de La Laguna, E-38205 La Laguna, Tenerife, Spain
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Abstract

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We present the IACOB spectroscopic database, the largest homogeneous database of high-resolution, high signal-to-noise ratio spectra of Northern Galactic OB-type stars compiled up to date. The spectra were obtained with the FIES spectrograph attached to the Nordic Optical Telescope. We briefly summarize the main characeristics and present status of the IACOB, first scientific results, and some future plans for its extension and scientific exploitation.

Keywords

stars: early-typetechniques: spectroscopiccatalogsastronomical data bases: miscellaneous
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S272: Active OB stars: structure, evolution, mass loss, and critical limits , July 2010 , pp. 310 - 312
Copyright
Copyright © International Astronomical Union 2011

References

Barbá, R. H., Gamen, R., Arias, J. I., Morrell, N. et al. 2010, in: Rivinius, T. & Curé, M. (eds.), The Interferometric View on Hot Stars, Rev. Mexicana AyA Conference Series 38, p. 30Google Scholar
Cunha, K. & Lambert, D. L. 1992, ApJ, 399, 586CrossRefGoogle Scholar
Evans, C., Hunter, I., Smartt, S., Lennon, D. et al. 2008, The Messenger, 131, 25Google Scholar
Evans, C. J., Bastian, N., Beletsky, Y., Brott, I. et al. 2010, in: de Grijs, R. & Lépine, J. R. D. (eds.), Star clusters: basic galactic building blocks throughout time and space, IAU Symposium 266, p. 35Google Scholar
Maíz-Apellániz, J., Walborn, N. R., Galué, H. Á. & Wei, L. H. 2004, ApJS, 151, 103CrossRefGoogle Scholar
Puls, J., Urbaneja, M. A., Venero, R., Repolust, T. et al. 2005, A&A, 435, 669Google Scholar
Simón-Díaz, S. 2010, A&A 510, 22Google Scholar
Simón-Díaz, S., Herrero, A., Uytterhoeven, K., Castro, N. et al. 2010, ApJ (Letters), 720, L174CrossRefGoogle Scholar