La Cellule.

Bibliography of agriculture

Wirtembergische Geschichte,

1. Th. Von der Urzeit bis 1080.--2. Th. Hohenstaufenzeit. 1080-1268.--3. Th. Schluss des Mittelalters. 1269-1496.--4. Th. Vornehmlich im 16. Jahrhundert.

Das gelehrte Teutschland; oder, Lexicon der jetztlebenden teutschen schriftsteller,

"1.[-2.] nachtrag": v. 3, p. [593]-860.

The Albany law journal [microform].

Title from caption.

Kongeriget Norges ordentlige Stortings forhandlinger. [microform]

Title varies slightly.

Report and transactions.

Place of publication varies: <2000-> Plymouth.

Hygiea.

Imprint varies.

Minutes of proceedings of the Institution of Civil Engineers.

Vol. for 1844 issued without title.

Surgery, gynecology & obstetrics

Editor: 1905-<19> F.H. Martin

Archiv für hessische Geschichte und Altertumskunde.

Some ills. folded.

Research interests of the Air Force Office of Scientific Research.

"1 October 1991."

Federal Communications Commission reports : decisions, reports, and orders of the Federal Communications Commission of the United States /

Title varies slightly.

Treatment-seeking behavior and delay in children with severe malaria in Uganda: results of a Markov analysis

Thesis (Master's)--University of Washington, 2016-06

Erectile Dysfunction Drug Use, Risk Behavior, and Sexually Transmitted Diseases

Thesis (Master's)--University of Washington, 2016-06

Diffuse optical light in galaxy clusters. I. Abell 3888

We are undertaking a program to measure the characteristics of the intracluster light ( ICL; total flux, profile, color, and substructure) in a sample of 10 galaxy clusters with a range of cluster mass, morphology, and redshift. We present here the methods and results for the first cluster in that sample, A3888. We have identified an ICL component in A3888 in V and r that contains 13% +/- 5% of the total cluster light and extends to 700 h(70)(-1) kpc (similar to 0.3r(200)) from the center of the cluster. The ICL color in our smallest radial bin is V - r 0.3 +/- 0.1, similar to the central cluster elliptical galaxies. The ICL is redder than the galaxies at 400 h(70)(-1) kpc < r < 700 h(70)(-1) kpc, although the uncertainty in any one radial bin is high. Based on a comparison of V - r color with simple stellar models, the ICL contains a component that formed more than 7 Gyr ago ( at z less than 1) with a high-metallicity ( 1.0 Z(circle dot) < Z(ICL) less than or similar to 2.5 Z(circle dot)) and a more centralized component that contains stars formed within the past 5 Gyr ( at z similar to 1). The profile of the ICL can be roughly fitted by a shallow exponential in the outer regions and a steeper exponential in the central region. We also find a concentration of diffuse light around a small group of galaxies 1.4 h(70)(-1) Mpc from the center of the cluster. In addition, we find three low surface brightness features near the cluster center that are blue ( V - r 0.0) and contain a total flux of 0.1M*. Based on these observations and X-ray and galaxy morphology, we suggest that this cluster is entering a phase of significant merging of galaxy groups in the core, whereupon we expect the ICL fraction to grow significantly with the formation of a cD galaxy, as well as the infall of groups.