Lee, Joseph H.

John J. Brice as I knew Him. Recollections of army career officer and music instructor, Joseph Lee about a young army recruit, John Brice, stationed at Camp Furlong in Columbus, New Mexico and later becoming in charge of ROTC at Howard University.https://dh.howard.edu/og_manusripts/1015/thumbnail.jp

Peggy H. Lee

A Virginia native and graduate of Virginia Tech, Peggy H. Lee began her career in restaurant management, but soon switched to school food service. She first worked as a supervisor of twenty-two schools in the Norfolk school system and then became the nutritionist for Virginia Beach Schools. From Virginia Beach she moved to Norfolk as a supervisor and then took the director’s position in Chesapeake. After thirty years of service she retired and now works for the National Dairy Council.https://egrove.olemiss.edu/icn_ohistories/1080/thumbnail.jp

Lee County 4-H Delegates

Lee County 4-H Delegates on Lee Hall stepshttps://scholarsjunction.msstate.edu/ua-photo-collection/9140/thumbnail.jp

Letter, S. H. Pope to W. H. Lee; 2/19/1865

Letter, Samuel H. Pope in Shuqualak, Mississippi, to William Hollinshed Lee, at the Officer\u27s Hospital in Uniontown, Alabama, expressing his desire for Lee to visit him at his boarding house. Sims was wounded and captured. Pope sympathizes with Lee\u27s unpleasant experience in the hospital. General Stephen D. Lee and Regina Harrison had a \u27\u27grand affair\u27\u27 of a wedding, and \u27\u27Maj. Blewitt gave them a large Confederate party the following evening.\u27\u27 Pope doesn\u27t believe that war time is the right time to get married. 1865.https://scholarsjunction.msstate.edu/mss-san-lee-sar-papers/1003/thumbnail.jp

Letter, S. H. Pope to W. H. Lee; 1/8/1865

Letter, Samuel H. Pope in Shuqualak, Mississippi, to William Hollinshed Lee, at the Officer\u27s Hospital in Uniontown, Alabama. Pope is stationed in Shuqualak as Purchasing Commissary. He invites Lee to visit Columbus and mentions that he can stay with Mrs. Morrow (Pope\u27s mother-in-law) and \u27\u27Miss Clodie\u27\u27 (Clotille Morrow). He wonders if Lee can work out a transfer to the hospital in Columbus. \u27\u27All excitement from Raids has subsided.\u27\u27 Sam Battle Fort was shot through both shoulders in November and was \u27\u27unable to push on a coat.\u27\u27 Pope explains why didn\u27t receive his recent mail in a timely way; when he telegraphed Lee, he had \u27\u27just returned from a tour of inspection on horse back, through the interior of the state.\u27\u27 1865.https://scholarsjunction.msstate.edu/mss-san-lee-sar-papers/1002/thumbnail.jp

My Friend—Lee H. Lytton

Tribute to Lee H. Lytton, a professor at St. Mary\u27s University School of Law in San Antonio, Texas

Sophia Lee, Flute

Lensky\u27s Aria from the opera Eugen Onegin, Op. 24 / Peter Tchaikovsky; Flute Sonata Undine, Op. 167 / Carl Reinecke; Sonata for Flute, Violin and Piano, H.254 / Bohuslav Martin

Infrared emission from ultracompact H II regions

Models of circumstellar dust shells around ultracompact (UC) H II regions were constructed that accurately fit the observed IR flux distributions. The models assume spherically symmetric dust shells illuminated by stars whose bolometric luminosity is inferred from the integrated FIR flux densities. Assuming ionization by a single zero age main sequence (ZAMS) star, the relations of Panagia were used to infer the stellar radius and effective temperature for a given luminosity. The grain mixture in the dust shell consists of bare graphite and silicate grains with the optical properties of Draine and Lee and the size distribution of Mathis et al. The computer code of Wolfire et al was used to solve the radiative transfer equations through a spherical dust shell. The model provides monochromatic luminosities, dust temperatures, and opacities through the shell. Aside from the stellar and dust properties, the only other input parameters to the model are the distance to the shell, the form of its density distribution, and its outer radius. Predictions of the model are compared with observations of a typical UC H II region and the run of dust temperature with radius and the optical depth with frequency are discussed