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20142021
most citedCHAOS I: Direct Chemical Abundances for HII Regions in NGC 628

181 citations · 756 across the 11 of their papers we have counts for

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11 papers · 1 filter

astro-ph.GA2021

Direct Far-Infrared Metal Abundances (FIRA) I: M101

C. Lamarche, J. D. Smith, K. Kreckel +12

Accurately determining gas-phase metal-abundances within galaxies is critical as metals strongly affect the physics of the interstellar medium (ISM). To date, the vast majority of…

astro-ph.GA201750 cited

Thermal Pressure in the Cold Neutral Medium of Nearby Galaxies

R. Herrera-Camus, A. Bolatto, M. Wolfire +14

Dynamic and thermal processes regulate the structure of the multi-phase interstellar medium (ISM), and ultimately establish how galaxies evolve through star formation. Thus, to con…

astro-ph.GA2016104 cited

Space Telescope and Optical Reverberation Mapping Project VI: reverberating Disk Models for NGC 5548

D. Starkey, Keith Horne, M. M. Fausnaugh +90

We conduct a multiwavelength continuum variability study of the Seyfert 1 galaxy NGC 5548 to investigate the temperature structure of its accretion disk. The 19 overlapping continu…

astro-ph.GA2016112 cited

The Spatially Resolved [CII] Cooling Line Deficit in Galaxies

J. D. T. Smith, Kevin Croxall, Bruce Draine +17

We present [CII] 158um measurements from over 15,000 resolved regions within 54 nearby galaxies of the KINGFISH program to investigate the so-called [CII] "line cooling deficit" lo…

astro-ph.GA2015181 cited

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…

astro-ph.GA2014115 cited

Dust continuum emission as a tracer of gas mass in galaxies

Brent A. Groves, Eva Schinnerer, Adam Leroy +8

We use a sample of 36 galaxies from the KINGFISH (Herschel IR), HERACLES (IRAM CO), and THINGS (VLA HI) surveys to study empirical relations between Herschel infrared (IR) luminosi…