Standing statue of the Celestial Worthy of the Great Unity, Savior from Suffering (Taiyi Jiuku tianzun)

H: 3 ft. 6 1/64 in.; gilt bronze

Letters on the condition of the poor : addressed to Alexander Henry, Esq., containing a vindication of poor laws and benevolent societies, proofs of the injustice of the general censure of the poor for extravagance, dissipation, etc., instances of intense suffering in Philadelphia ... /

Goldsmiths'-Kress no. 29122.

Lachrymae ecclesiae; the Anglican reformed church and her clergy in the days of their destitution and suffering during the great rebellion in the seventeenth century.

Mode of access: Internet.

Christ dying and drawing sinners to himself, or, A survey of our Saviour in his soul-suffering, his loveliness in his death, and the efficacy thereof ... delivered in sermons on the Gospel according to John ... /

Mode of access: Internet.

Memoir of Hannah Hobbie, or, Christian activity, and triumph in suffering /

Mode of access: Internet.

Biological control of spotted and diffuse knapweeds.

"Issued December 1994"--P. [2].

The suffering Savior : or, Meditations on the last days of Christ.

Tr. of: Der leidende Christus.

Selections from the Epistles, &c. of William Bennit : an early minister of the Gospel in the Society of Friends, who, after suffering long and patiently ... : a memoir of his religious experience and character.

Mode of access: Internet.

Comparing the concentration of calcium hydroxide in the diffuse double layer by modeling and experiment

The leaching of elements from the surface of charged fly ash particles is known to be an unsteady process. The mass transfer resistance provided by the diffuse double layer has been quantified as one of the reasons for this delayed leaching. In this work, a model based on mass transfer principles for predicting the concentration of calcium hydroxide in the diffuse double layer is presented. The significant difference between predicted calcium hydroxide concentration and the experimentally measured is explained.

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.