Issue |
A&A
Volume 448, Number 2, March III 2006
|
|
---|---|---|
Page(s) | 513 - 524 | |
Section | Extragalactic astronomy | |
DOI | https://doi.org/10.1051/0004-6361:20053788 | |
Published online | 24 February 2006 |
First detection of Lyman continuum escape from a local starburst galaxy
I. Observations of the luminous blue compact galaxy Haro 11 with the Far Ultraviolet Spectroscopic Explorer (FUSE)
1
Dept. of Astronomy and Space Physics, Box 515, 75120 Uppsala, Sweden e-mail: [nils.bergvall;erik.zackrisson]@astro.uu.se
2
Department of Physics and Astronomy, Johns Hopkins University, 3400 North Charles Street, Baltimore, MD 21218, USA e-mail: bg@pha.jhu.edu
3
Instituto de Astrofisica de Andalucia, Granada, Spain e-mail: pepa@iaa.es
4
Stockholm Observatory, SCFAB, 106 91 Stockholm, Sweden e-mail: ostlin@astro.su.se
Received:
7
July
2005
Accepted:
2
November
2005
Context.The dominating reionization source in the young universe has not yet
been identified. Possible candidates include metal poor dwarf galaxies with
starburst properties.Aims.We selected an extreme starburst dwarf, the Blue Compact
Galaxy Haro 11, with the aim of determining the Lyman continuum
escape fraction from UV spectroscopy.Methods.Spectra of Haro 11 were obtained with the Far Ultraviolet
Spectroscopic Explorer (FUSE). A weak signal shortwards of the Lyman break is
identified as Lyman continuum (LyC) emission escaping from the ongoing
starburst. From profile fitting to weak metal lines we derive column densities
of the low ionization species. Adopting a metallicity typical of the H II
regions of Haro 11, these data correspond to a hydrogen column density of
~1019cm-2. This relatively high value indicates that most of the
LyC photons escape through transparent holes in the interstellar medium. We then
use spectral evolutionary models to constrain the escape fraction of the
produced LyC photons.Results.Assuming a normal Salpeter initial mass function we obtain a Lyman continuum escape fraction
of 4–10%. We argue that in a
hierarchical galaxy formation scenario, the upper limit we derive for the escape
rate allows for a substantial contribution to cosmic reionization by starburst
dwarf galaxies at high redshifts.
© ESO, 2006
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