Modeling the ISM properties of metal-poor galaxies and gamma-ray burst hosts
Recent research has suggested that long-duration gamma-ray bursts (LGRBs) occur preferentially in low-metallicity environments, but the exact nature of this correlation is currently a matter of intense debate. We use the newest generation of the Starburst99/Mappings code to generate an extensive suite of cutting-edge stellar population synthesis models, covering a wide range of physical parameters specifically tailored for modeling the ISM environments of metal-poor galaxies and LGRB host...[Show more]
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|Source:||Low-metallicity Star Formation|
|01_Levesque_Modeling_the_ISM_properties_of_2008.pdf||277.75 kB||Adobe PDF||Request a copy|
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