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Gerald Cecil

Researcher at University of North Carolina at Chapel Hill

Publications -  102
Citations -  6233

Gerald Cecil is an academic researcher from University of North Carolina at Chapel Hill. The author has contributed to research in topics: Galaxy & Active galactic nucleus. The author has an hindex of 38, co-authored 102 publications receiving 5757 citations. Previous affiliations of Gerald Cecil include Institute for Advanced Study & University of Hawaii.

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Galactic Winds

TL;DR: Galactic winds are the primary mechanism by which energy and metals are recycled in galaxies and are deposited into the intergalactic medium New observations are revealing the ubiquity of this process, particularly at high redshift as discussed by the authors.
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The SAMI Galaxy Survey: Instrument specification and target selection

Julia J. Bryant, +67 more
TL;DR: The SAMI Galaxy Survey as discussed by the authors is a 3-year survey of 3400 galaxies with the Sydney-AAO Multi-Object Integral Field Spectrograph (SAMI) on the Anglo-Australian Telescope (AAT).
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Are the Narrow-Line Regions in Active Galaxies Dusty and Radiation Pressure Dominated?

TL;DR: In this article, dust and the radiation pressure acting upon it provide the controlling factor in moderating the density, excitation, and surface brightness of photoionized narrow line regions (NLRs) structures.
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Jet- and wind-driven ionized outflows in the superbubble and star-forming disk of NGC 3079

TL;DR: In this paper, WFPC2 images are presented that span the inner ~19 kpc diameter of the edge-on galaxy NGC 3079; they are combined with optical, emission-line imaging spectrophotometry and VLA images of radio polarization vectors and rotation measures.
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The nuclear superbubble of ngc 3079

TL;DR: In this article, the authors used the Hawaii Imaging Fabry-Perot Interferometer (HIFI) at the CFH 3.6 m telescope to map H-alpha + (N II) lambda-lambda 6548, 6583 emission-line profiles across the entire edge-on, nearby SBc galaxy NGC 3079, with resolution 70 km/s and subarcsecond sampling.