Making the Connection between Feedback and Spatially Resolved Emission Line 
Diagnostics

Pellegrini, Eric; Drory, Niv; Lopez, Laura A.; Simon, Josh; Jones, Amy; Kreckel, Kathryn; Avila, Vladimir; Tuttle, Sarah; Yan, Renbin; Blanc, Guillermo; Kollmeier, Juna

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Journal Article

Making the Connection between Feedback and Spatially Resolved Emission Line Diagnostics

MPS-Authors

Pellegrini, Eric
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Drory, Niv
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Lopez, Laura A.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Simon, Josh
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Jones, Amy
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Kreckel, Kathryn
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Avila, Vladimir
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Tuttle, Sarah
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Yan, Renbin
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Blanc, Guillermo
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Kollmeier, Juna
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

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https://ui.adsabs.harvard.edu/abs/2019BAAS...51c.406P
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Citation

Pellegrini, E., Drory, N., Lopez, L. A., Simon, J., Jones, A., Kreckel, K., et al. (2019). Making the Connection between Feedback and Spatially Resolved Emission Line Diagnostics. Bulletin of the American Astronomical Society, 51.

Cite as: https://hdl.handle.net/21.11116/0000-0005-D01C-1

Abstract

We argue that crucial progress in the coming decade will depend on the ability to obtain spatially resolved spectroscopic observations of HII regions for reliable instantaneous measurements of their physical conditions, with full galactic coverage to obtain a population sample with line sensitivities significantly deeper than past efforts.