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Mapping the Properties of Blue Compact Dwarf Galaxies by Means of Integral Field Spectroscopy

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Dwarf Galaxies: Keys to Galaxy Formation and Evolution

Part of the book series: Astrophysics and Space Science Proceedings ((ASSSP))

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Abstract

Blue Compact Dwarf (BCD) galaxies are metal-poor and gas-rich systems undergoing intense, spatially extended star-forming activity. These galaxies offer a unique opportunity to investigate dwarf galaxy formation and evolution, and probe violent star formation and its implications on the chemical, dynamical and structural properties of low-mass extragalactic systems near and far. Several fundamental questions in BCD research, such as their star formation histories and the mechanisms that control their cyclic starburst activity, are still far from well understood. In order to improve our understanding on BCD evolution, we are carrying out a comprehensive Integral Field Spectroscopic (IFS) survey of a large sample of BCDs. Integral Field Unit (IFU) spectroscopy provides simultaneously spectral and spatial information, allowing, in just one shot, to study the morphology and evolutionary status of the stellar component, and the physical properties of the warm interstellar medium (e.g., extinction, chemical abundances, kinematics). This ongoing IFS survey will supply much needed local templates that will ease the interpretation of IFS data for intermediate and high-redshift star-forming galaxies.

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Notes

  1. 1.

    VIRUS-P is the prototype instrument for VIRUS, a massively replicated IFU, made of 150 units, which will be installed on the 9.2 m Hobby-Eberly Telescope [6].

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Acknowledgements

P. Weilbacher acknowledges support by the German Verbundforschung through the MUSE/D3Dnet project (grant 05A08BA1). P. Papaderos is supported by Ciencia 2008 Contract, funded by FCT/MCTES (Portugal) and POPH/FSE (EC). B. García-Lorenzo acknowledges support from the Instituto de Astrofísica de Canarias and the Spanish Ministerio de Ciencia e Innovación (AYA2009-12903 and the Ramón y Cajal program).

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Correspondence to L. M. Cairós .

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© 2012 Springer-Verlag Berlin Heidelberg

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Cairós, L.M., Caon, N., Weilbacher, P., Papaderos, P., García-Lorenzo, B. (2012). Mapping the Properties of Blue Compact Dwarf Galaxies by Means of Integral Field Spectroscopy. In: Papaderos, P., Recchi, S., Hensler, G. (eds) Dwarf Galaxies: Keys to Galaxy Formation and Evolution. Astrophysics and Space Science Proceedings. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-22018-0_24

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  • DOI: https://doi.org/10.1007/978-3-642-22018-0_24

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  • Print ISBN: 978-3-642-22017-3

  • Online ISBN: 978-3-642-22018-0

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