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Determination of the OB Stellar Population of IZw18 on the Basis of its Hγ and Hδ Absorption lines
Published online by Cambridge University Press: 25 May 2016
Abstract
On the basis of new spectroscopic observations of the blue compact dwarf galaxy IZw18 in the narrow spectral range between 4000Å and 4500Å absorption components of Hγ and Hδ lines were discovered. Equivalent widths of Hγ and Hδ lines have been measured. From available data the OB population of IZw18 was analyzed.
- Type
- IV. AGN Related Phenomena
- Information
- Symposium - International Astronomical Union , Volume 194: Activity in Galaxies and Related Phenomena , 1999 , pp. 444 - 447
- Copyright
- Copyright © Astronomical Society of the Pacific 1999