# Large-scale shock-ionized and photo-ionized gas in M83: the impact of star formation

@article{Hong2011LargescaleSA,
title={Large-scale shock-ionized and photo-ionized gas in M83: the impact of star formation},
author={Sungryong Hong and Daniela Calzetti and Michael A. Dopita and William P. Blair and Bradley C. Whitmore and Bruce Balick and Howard E. Bond and Marcella Carollo and Michael John Disney and Jay. A. Frogel and Donald B. Hall and Jon A. Holtzman and Randy A. Kimble and Patrick McCarthy and Robert W. O’Connell and Francesco Paresce and Abhijit Kumar Saha and Joseph I. Silk and John Terry Trauger and Alistair R. Walker and Rogier A. Windhorst and Erick T. Young and Max J. Mutchler},
journal={arXiv: Cosmology and Nongalactic Astrophysics},
year={2011}
}
• Published 11 February 2011
• Physics
• arXiv: Cosmology and Nongalactic Astrophysics
We investigate the ionization structure of the nebular gas in M83 using the line diagnostic diagram, [O III](5007 \degA)/H{\beta} vs. [S II](6716 \deg A+6731 \deg A)/H{\alpha} with the newly available narrowband images from the Wide Field Camera 3 (WFC3) of the Hubble Space Telescope (HST). We produce the diagnostic diagram on a pixel-by-pixel (0.2" x 0.2") basis and compare it with several photo- and shock-ionization models. For the photo-ionized gas, we observe a gradual increase of the log…
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## References

SHOWING 1-10 OF 66 REFERENCES
Further Spectroscopy of the Diffuse Ionized Gas in NGC 891 and Evidence for a Secondary Source of Ionization
Two long-slit spectra of the diffuse ionized gas (DIG) in NGC 891 are presented. The first reveals variations parallel to the major axis in emission-line ratios in the halo gas at z = 700 pc. It is
The Ionized Gas in Local Starburst Galaxies: Global and Small-Scale Feedback from Star Formation*
• Physics
• 2003
The small- and intermediate-scale structure and the fraction of the interstellar medium (ISM) ionized by nonradiative processes are investigated in a small sample of four local starburst galaxies,
NGC 839: SHOCKS IN AN M82-LIKE SUPERWIND
• Physics
• 2010
We present observations of NGC 839 made with the Wide Field Spectrograph (WiFeS) on the ANU 2.3m telescope. Our data cover a region 25 00 × 60 00 at a spatial resolution of � 1.5 00 . The long axis
Theoretical models of interstellar shocks. I - Radiative transfer and UV precursors
• Physics
• 1979
We construct theoretical models of interstellar radiative shocks, with special attention to the transfer of ionizing radiation. These models are ''self-consistent'' in the sense that the emergent
SUPERNOVA REMNANTS AND THE INTERSTELLAR MEDIUM OF M83: IMAGING AND PHOTOMETRY WITH THE WIDE FIELD CAMERA 3 ON THE HUBBLE SPACE TELESCOPE
• Physics
• 2010
We present Wide Field Camera 3 images taken with the Hubble Space Telescope within a single field in the southern grand design star-forming galaxy M83. Based on their size, morphology, and photometry
Far-ultraviolet observations of the supernova remnant N49 using the Hopkins Ultraviolet Telescope
• Physics
• 1992
The Hopkins Ultraviolet Telescope has been used to obtain the first sub-Lyman-alpha spectrum of an extragalactic SNR, N49, in the LMC. Emission from O VI 1032, 1038 has been detected in this spectral
Hubble Space Telescope/WFPC2 and VLA Observations of the Ionized Gas in the Dwarf Starburst Galaxy NGC 4214
• Physics
• 2000
We present new Hα and [O III] λ5007 narrowband images of the starbursting dwarf galaxy NGC 4214, obtained with the Wide Field and Planetary Camera (WFPC2) on board the Hubble Space Telescope (HST),
Modeling the Pan-Spectral Energy Distribution of Starburst Galaxies. III. Emission Line Diagnostics of Ensembles of Evolving H II Regions
• Physics
• 2006
We build, as far as theory will permit, self-consistent model H II regions around central clusters of aging stars. These produce strong emission line diagnostics applicable to either individual H II
Mapping Large-Scale Gaseous Outflows in Ultraluminous Infrared Galaxies with Keck II ESI Spectra: Spatial Extent of the Outflow
The kinematics of neutral gas and warm ionized gas have been mapped across ultraluminous starburst galaxies using the Na I λλ5890, 5896 absorption-line and Hα emission-line profiles, respectively, in
The MAPPINGS III Library of Fast Radiative Shock Models
• Physics
• 2008
We present a new library of fully-radiative shock models calculated with the MAPPINGS III shock and photoionization code. The library consists of grids of models with shock velocities in the range