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Leo P: How Many Metals can a Very Low-Mass, Isolated Galaxy Retain?
Kristen B. W. McQuinn, Evan D. Skillman, Andrew Dolphin +7
Leo P is a gas-rich dwarf galaxy with an extremely low gas-phase oxygen abundance (3% solar). The isolated nature of Leo P enables a quantitative measurement of metals lost solely…
Leo P: An Unquenched Very Low-Mass Galaxy
Kristen B. W. McQuinn, Evan D. Skillman, Andrew Dolphin +8
Leo P is a low-luminosity dwarf galaxy discovered through the blind HI Arecibo Legacy Fast ALFA (ALFALFA) survey. The HI and follow-up optical observations have shown that Leo P is…
CHAOS II: Gas-Phase Abundances in NGC 5194
Kevin V. Croxall, Richard W. Pogge, Danielle Berg +2
We have observed NGC5194 (M51a) as part of the CHemical Abundances of Spirals (CHAOS) project. Using the Multi Object Double Spectrographs (MODS) on the Large Binocular Telescope (…
CHAOS I: Direct Chemical Abundances for HII Regions in NGC 628
Danielle A. Berg, Kevin V. Croxall, Evan D. Skillman +3
The CHemical Abundances of Spirals (CHAOS) project leverages the combined power of the Large Binocular Telescope (LBT) with the broad spectral range and sensitivity of the Multi Ob…