Oxygen abundance - PowerPoint PPT Presentation

Mixing of metals in blue LSB galaxies ( or How one can measure their ages )

Mixing of metals in blue LSB galaxies ( or How one can measure their ages ). Yuri Shchekinov (Southern Federal U) Eduard Vorobyov (St. Marry U, S Fed U) Domink Bomans (AI RUB) Ralf-Jurgen Dettmar (AI RUB) Dmitry Bizyaev (New Mexico State U, Sternberg AI).

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374 views • 29 slides

COS Observations of the Chemical Composition of SNR LMC N132D France et al.

COS Observations of the Chemical Composition of SNR LMC N132D France et al. Ben Folsom and Sharlene Rubio. Background on Supernovae:. -Fe 56 is the most stable isotope inside a star, meaning it requires energy input for fusion or fission.

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288 views • 18 slides

References

Henry Lee (hlee@astro.umn.edu). Starbursts - From 30 Doradus to Lyman Break Galaxies, Cambridge. The Dwarf Starburst Galaxy NGC 1705 : New H II Region Element Abundances &amp; Reddening Variations Near the Center. Henry Lee &amp; Evan D. Skillman University of Minnesota.

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147 views • 1 slides

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