168 citations · 481 across the 11 of their papers we have counts for
11 papers
The SDSS-V Local Volume Mapper (LVM): Scientific Motivation and Project Overview
Niv Drory, Guillermo A. Blanc, Kathryn Kreckel +48
We present the Sloan Digital Sky Survey V (SDSS-V) Local Volume Mapper (LVM). The LVM is an integral-field spectroscopic survey of the Milky Way, Magellanic Clouds, and of a sample…
SIGNALS: I. Survey Description
L. Rousseau-Nepton, R. P. Martin, C. Robert +60
SIGNALS, the Star formation, Ionized Gas, and Nebular Abundances Legacy Survey, is a large observing program designed to investigate massive star formation and HII regions in a sam…
Astro2020 Science White Paper: Making the Connection between Feedback andSpatially Resolved Emission Line Diagnostics
E. W. Pellegrini, N. Drory, Guillermo A. B. +8
Crucial progress in our understanding of star formation and feedback will depend on the ability to obtain spatially resolved spectroscopic observations of \ion{H}{ii} regions, from…
Feedback in W49A diagnosed with radio recombination lines and models
M. R. Rugel, D. Rahner, H. Beuther +20
We present images of radio recombination lines (RRLs) at wavelengths around 17 cm from the star-forming region W49A to determine the kinematics of ionized gas in the THOR survey (T…
Dust emission at 8-mic and 24-mic as Diagnostics of HII Region Radiative Transfer
M. S. Oey, J. Lopez-Hernandez, J. A. Kellar +10
We use the Spitzer SAGE survey of the Magellanic Clouds to evaluate the relationship between the 8-mic PAH emission, 24-mic hot dust emission, and HII region radiative transfer. We…
The Radio Spectral Energy Distribution and Star Formation Rate Calibration in Galaxies
F. S. Tabatabaei, E. Schinnerer, M. Krause +17
We study the spectral energy distribution (SED) of the radio continuum emission from the KINGFISH sample of nearby galaxies to understand the energetics and origin of this emission…
The Ionized Gas in Nearby Galaxies as Traced by the [NII] 122 and 205 μm Transitions
R. Herrera-Camus, A. Bolatto, J. D. Smith +20
The [NII] 122 and 205 μm transitions are powerful tracers of the ionized gas in the interstellar medium. By combining data from 21 galaxies selected from the Herschel KINGFISH and…
A milestone toward understanding PDR properties in the extreme environment of LMC-30Dor
M. Chevance, S. C. Madden, V. Lebouteiller +11
More complete knowledge of galaxy evolution requires understanding the process of star formation and interaction between the interstellar radiation field and the interstellar mediu…
The dust properties and physical conditions of the interstellar medium in the LMC massive star forming complex N11
M. Galametz, S. Hony, M. Albrecht +19
We combine Spitzer and Herschel data of the star-forming region N11 in the Large Magellanic Cloud to produce detailed maps of the dust properties in the complex and study their var…
Towards A Removal of Temperature Dependencies from Abundance Determinations
Kevin V. Croxall, J. D. Smith, B. R. Brandl +16
The metal content of a galaxy is a key property for distinguishing between viable galaxy evolutionary scenarios, and it strongly influences many of the physical processes in the in…
Single-Star HII Regions as a Probe of Massive Star Spectral Energy Distributions
Jordan Zastrow, M. S. Oey, E. W. Pellegrini
The shape of the OB-star spectral energy distribution is a critical component in many diagnostics of the ISM and galaxy properties. We use single-star HII regions from the LMC to q…