Testimony of John J. Lawler Before the Commission on the Future of Worker-Management Relations

Testimony_Lawler_022494.pdf: 224 downloads, before Oct. 1, 2020

Divided House Revisited, Report to the spring meeting of Council, May 6, 1970

https://egrove.olemiss.edu/aicpa_assoc/2071/thumbnail.jp

Letters from John Lawler to Members of Council, May 12, 1972 and October 20, 1972

https://egrove.olemiss.edu/aicpa_assoc/1946/thumbnail.jp

Speech to Association of CPA Examiners, Hotel Americana, Bal Harbour, Florida, October 3, 1964

https://egrove.olemiss.edu/aicpa_exam/1187/thumbnail.jp

Improved Co I Log(gf) Values and Abundance Determinations in the Photospheres of the Sun and Metal-Poor Star HD 84937

New emission branching fraction measurements for 898 lines of the first spectrum of cobalt (Co I) are determined from hollow cathode lamp spectra recorded with the National Solar Observatory 1 m Fourier transform spectrometer on Kitt Peak, AZ and a high-resolution echelle spectrometer. Published radiative lifetimes from laser induced fluorescence measurements are combined with the branching fractions to determine accurate absolute atomic transition probabilities for the 898 lines. Hyperfine structure (hfs) constants for levels of neutral Co in the literature are surveyed and selected values are used to generate complete hfs component patterns for 195 transitions of Co I. These new laboratory data are applied to determine the Co abundance in the Sun and metal-poor star HD 84937, yielding log epsilon(Co) = 4.955 +/- 0.007 (sigma = 0.059) based on 82 Co I lines and log epsilon(Co) = 2.785 +/- 0.008 (sigma = 0.065) based on 66 Co I lines, respectively. A Saha or ionization balance test on the photosphere of HD 84937 is performed using 16 UV lines of Co II, and good agreement is found with the Co I result in this metal-poor ([Fe I/H] = -2.32, [Fe II/H] = -2.32) dwarf star. The resulting value of [Co/Fe]= +0.14 supports a rise of Co/Fe at low metallicity that has been suggested in other studies.NASA NNX10AN93GNSF AST-1211055, AST-1211585McDonald Observator

Inspire: the confluence of art & design

Inspire: The Confluence of Art & Design seeks to untangle the inextricable link between graphic design and art. Graphic design has always been seen simply as an informational or sales tool; rarely is it seen as art. The work presented in this show illustrates that works created with typography can, in fact, be one and the same

General Report of the Board of Directors, May 4, 1970

https://egrove.olemiss.edu/aicpa_assoc/2035/thumbnail.jp

Improved Log(gf) Values for Lines of Ti I and Abundance Determinations in the Photospheres of the Sun and Metal-Poor Star HD 84937 (Accurate Transition Probabilities for Ti I)

New atomic transition probability measurements for 948 lines of Ti I are reported. Branching fractions from Fourier transform spectra and from spectra recorded using a 3 m echelle spectrometer are combined with published radiative lifetimes from laser-induced fluorescence measurements to determine these transition probabilities. Generally good agreement is found in comparisons to the NIST Atomic Spectra Database. The new Ti I data are applied to re-determine the Ti abundance in the photospheres of the Sun and metal-poor star HD 84937 using many lines covering a range of wavelength and excitation potential to explore possible non-local thermal equilibrium effects. The variation of relative Ti/Fe abundance with metallicity in metal-poor stars observed in earlier studies is supported in this study.NSF AST-1211055, AST-0908978, AST-1211585NSF REU grant AST-1004881ESO Science Archive Facility 073.D-0024, 266.D-5655NASA NAS 5-26555Astronom