... G. J. Ferland, K. T. Korista, and D. A. Verner . ... The development of Cloudy is a three-pronged effort requiring advances in the underlying atomic data base, the numerical and computational methods used in the simulation, culminating in the application to astronomical problems. ... Finally, rescaled OP oscillator strengths were used to compile a complete set of data for 5971 resonance lines (Verner, Verner, & Ferland 1996). ... Verner, D. A., Verner, E. M., & Ferland, G. J. 1996, Atomic Data Nucl....

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... From Ice Skater Physics to Star Birth in HII Regions. ... The group will meet at the Rte579 Astronomy Events for 2006 Edited by Barlow Bob Feb 20 - 25 Winter Star Party, Florida Keys, FL http : //www.scas.org/ Zombie Party, Atlanta, GA http ://www.atlan taastronomy.org/ Apr 28 ґ May 2 Delmarva Star Gaze Star Party, Tuckahoe State Park, MD http ://www.delmarvastargaze rs.org/archive/sg2006/sg2006.html South Jersey Spring Star Party, Belleplain State Forest, NJ http :// ...

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• http://www.princetonastronomy.org/newsletters/11_2005sidereal.pdf
• http://www.princetonastronomy.org/newsletters/06_2007sidereal.pdf
• http://www.princetonastronomy.org/newsletters/03_2006sidereal.pdf

... The Thickness of Stellar Disks in Early-type Galaxies E. M. Chudakova* and O. K. Sil'chenko ** Sternberg Astronomical Institute, Lomonosov Moscow State University, Moscow, Russia Received August 19, 2013; in final form, October 30, 2013 Abstract--We suggest and justify a new photometric method enabling the derivation of the relative thickness of a galactic disk from the two-dimensional surface-brightness distribution of the galaxy in the plane of the sky. ... The galaxies are non-interacting. ...

206. TUI:Version History