HII Regions

Resolved HII Regions with SIGNALS featured image

Resolved HII Regions with SIGNALS

Nebular emission lines are some of our most powerful tools for studying galaxies. From a handful of bright lines, we routinely estimate properties of star-forming regions (and …

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Ray Garner
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M101 Group: Galaxy Evolution in a Nearby Laboratory featured image

M101 Group: Galaxy Evolution in a Nearby Laboratory

I have focused on the M101 Group since graduate school. Because it is only a few megaparsecs away, this small, isolated galaxy group gives us a detailed look at how spiral galaxies …

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Ray Garner
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HII Region Filling Factors in NGC 628: Luminosity-Size Relation and Connection with PAH Emission featured image

HII Region Filling Factors in NGC 628: Luminosity-Size Relation and Connection with PAH Emission

*Aims.* Understanding the internal structure of H II regions is fundamental to constraining star-formation processes in galaxies. We investigate how the *filling factor* (FF) …

lorena-araguete-riesco
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SIGNALS of Giant HII Regions: A Spatially Resolved Analysis of NGC 604 featured image

SIGNALS of Giant HII Regions: A Spatially Resolved Analysis of NGC 604

Observing giant H II regions at fine spatial scales uncovers detailed structures and reveals variations in ionization, abundance, and dynamical properties of ionized gas and the …

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Ray Garner
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SIGNALS of Giant HII Regions: A Spatially Resolved Analysis of NGC 604 featured image

SIGNALS of Giant HII Regions: A Spatially Resolved Analysis of NGC 604

A 5-minute oral presentation delivered to the American Astronomical Society. This covers a recent completed paper on the spatially resolved data of NGC 604 as part of the SIGNALS …

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Ray Garner
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Optical Strong Line Ratios Cannot Distinguish Between Stellar Populations and Accreting Black Holes at High Ionization Parameters and Low Metallicities featured image

Optical Strong Line Ratios Cannot Distinguish Between Stellar Populations and Accreting Black Holes at High Ionization Parameters and Low Metallicities

High-redshift observations from JWST indicate that optical strong line ratios do not carry the same constraining power as they do at low redshifts. Critically, this prevents a …

nikko-j.-cleri
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Poster: SIGNALS of Giant HII Regions: Resolved Ionization & Abundance Properties of NGC 604 featured image

Poster: SIGNALS of Giant HII Regions: Resolved Ionization & Abundance Properties of NGC 604

A poster presentation about my work investigating the spatially-resolved properties of NGC 604.

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Ray Garner
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AggieSTAAR: Introduction to HII Regions featured image

AggieSTAAR: Introduction to HII Regions

This talk was given as part of a weekly lunch talk for the undergraduates in the Aggie Scholarships for Technology Advancements in Astronomical Research (AggieSTAAR) program. In …

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Ray Garner
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The SIGNALS from HII Regions featured image

The SIGNALS from HII Regions

An invited review talk at the SIGNALS workshop about HII regions, pockets of gas ionized by hot stars. In this talk, I give an overview of the work that has been done about HII …

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Ray Garner
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Explaining the Abundance-Ionization Correlation in HII Regions with NGC 628 featured image

Explaining the Abundance-Ionization Correlation in HII Regions with NGC 628

An invited presentation about my work investigating the correlation between the ionization parameter and oxygen abundance in NGC 628.

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Ray Garner
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