Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 421, Issue 2, Pages 1043-1063Publisher
OXFORD UNIV PRESS
DOI: 10.1111/j.1365-2966.2012.20439.x
Keywords
stars: Wolf-Rayet; galaxies: evolution; galaxies: star formation; galaxies: stellar content
Categories
Funding
- Alfred P. Sloan Foundation
- National Science Foundation
- US Department of Energy
- National Aeronautics and Space Administration
- Japanese Monbukagakusho
- Max Planck Society
- Higher Education Funding Council for England
- American Museum of Natural History
- Astrophysical Institute Potsdam
- University of Basel
- University of Cambridge
- Case Western Reserve University
- University of Chicago
- Drexel University, Fermilab
- Institute for Advanced Study
- Japan Participation Group
- Johns Hopkins University
- Joint Institute for Nuclear Astrophysics
- Kavli Institute for Particle Astrophysics and Cosmology
- Korean Scientist Group
- Chinese Academy of Sciences (LAMOST)
- Los Alamos National Laboratory
- Max-Planck-Institute for Astronomy (MPIA)
- Max-Planck-Institute for Astrophysics (MPA)
- New Mexico State University
- Ohio State University
- University of Pittsburgh
- University of Portsmouth
- Princeton University
- United States Naval Observatory
- University of Washington
- Particle Physics and Astronomy Research Council (PPARC)
- Joint Astronomy Centre Hawaii
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We present a sample of 2865 emission-line galaxies with strong nebular He II lambda 4686 emissions in the Sloan Digital Sky Survey Data Release 7 and use this sample to investigate the origin of this line in star-forming galaxies. We show that star-forming galaxies and galaxies dominated by an active galactic nucleus form clearly separated branches in the He II lambda 4686/H beta versus [N-II]lambda 6584/H alpha diagnostic diagram and derive an empirical classification scheme which separates the two classes. We also present an analysis of the physical properties of 189 star-forming galaxies with strong He II lambda 4686 emissions. These star-forming galaxies provide constraints on the hard ionizing continuum of massive stars. To make a quantitative comparison with observation, we use photoionization models and examine how different stellar population models affect the predicted He II lambda 4686 emission. We confirm previous findings that the models can predict He II lambda 4686 emission only for instantaneous bursts of 20 per cent solar metallicity or higher, and only for ages of similar to 4-5 Myr, the period when the extreme-ultraviolet continuum is dominated by emission from Wolf-Rayet stars. We find, however, that 83 of the star-forming galaxies (40 per cent) in our sample do not have Wolf-Rayet features in their spectra despite showing strong nebular He II lambda 4686 emission. We discuss possible reasons for this and possible mechanisms for the He II lambda 4686 emission in these galaxies.
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