Abstract
We analyze spectra of blue compact dwarf galaxies from the Sloan Digital Sky Survey Data Release 7 with Hβλ4861 fluxes exceeding 10−14 erg s−1 cm−2. Nearly all galaxies in our sample show broad Wolf-Rayet (WR) emission in the blue region of the spectrum (the blue bump) consisting of an unresolved blend of NIII λ4640, HeII λ4686 emission lines. Broad CIV λ5808 emission (the red bump) is also detected in a few galaxies. We derive the numbers of early WC (WCE) and late WN (WNL) stars from the luminosities of the red and blue bumps, and the number of O stars from the luminosity of the Hβ emission line and compare the relative number of WR stars N(WR)/N(O+WR) with predictions from evolutionary synthesis models.
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Acknowledgements
The author warmly thanks the Organizing Committee for its kind hospitality and the European Astronomical Society for partial financial support. This work was partially supported by the Cosmomicrophysics program of the National Academy of Sciences and the National Space Agency of Ukraine.
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Agiienko, K. (2012). Wolf-Rayet Galaxies in SDSS DR7. 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_26
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DOI: https://doi.org/10.1007/978-3-642-22018-0_26
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