Proceedings.

Part of Nebraska Law Review, v. 20, 1941-(1966)

Estatutos de la Real Academia de Jurisprudencia teórico-práctica de San Fernando, de esta capital de la Habana : aprobados por el supremo gobierno en real órden de 16 de setiembre de 1841.

Mode of access: Internet.

The legal profession in Upper Canada in its early periods /

"Some of the matter contained in this work has already appeared in different form in addresses to various bar associations ... and in papers in legal publications ... or in other magazines."--Pref.

Proceedings of the ... annual meeting /

Imprint varies.

Proceedings and committee reports.

Vols. contain reports of the association and proceedings of the annual meetings, occasional special meetings; and midsummer meetings for 1938-1941.

Report of proceedings

List of places of meeting, etc., 1888-1922: 33d, 1921, p. [10]

Constitution and by-laws. 1898

Photocopy. Buffalo, Dennis, 1941

A general summary of the proceedings of the First Annual Meeting.

Includes Constitution and By-Laws of the Florida State Bar Association.

Year book /

Mode of access: Internet.

Transactions of the annual meeting.

Includes list of members.

Constitution and by-laws, list of members /

Mode of access: Internet.

Massive open star clusters using the VVV survey III. A young massive cluster at the far edge of the Galactic bar

Context. Young massive clusters are key to map the Milky Way’s structure, and near-infrared large area sky surveys have contributed strongly to the discovery of new obscured massive stellar clusters. Aims. We present the third article in a series of papers focused on young and massive clusters discovered in the VVV survey. This article is dedicated to the physical characterization of VVV CL086, using part of its OB-stellar population. Methods. We physically characterized the cluster using JHKS near-infrared photometry from ESO public survey VVV images, using the VVV-SkZ pipeline, and near-infrared K-band spectroscopy, following the methodology presented in the first article of the series. Results. Individual distances for two observed stars indicate that the cluster is located at the far edge of the Galactic bar. These stars, which are probable cluster members from the statistically field-star decontaminated CMD, have spectral types between O9 and B0 V. According to our analysis, this young cluster (1.0 Myr < age < 5.0 Myr) is located at a distance of 11+5-6 kpc, and we estimate a lower limit for the cluster total mass of (2.8+1.6-1.4) · 103 M⊙. It is likely that the cluster contains even earlier and more massive stars.

The Queensland study of melanoma : Environmental and genetic associations (Q-MEGA); Study design, baseline characteristics, and repeatability of phenotype and sun exposure measures

Cutaneous malignant melanoma (CMM) is a major health issue in Queensland, Australia, which has the world’s highest incidence. Recent molecular and epidemiologic studies suggest that CMM arises through multiple etiological pathways involving gene-environment interactions. Understanding the potential mechanisms leading to CMM requires larger studies than those previously conducted. This article describes the design and baseline characteristics of Q-MEGA, the Queensland Study of Melanoma: Environmental and Genetic Associations, which followed up 4 population-based samples of CMM patients in Queensland, including children, adolescents, men aged over 50, and a large sample of adult cases and their families, including twins. Q-MEGA aims to investigate the roles of genetic and environmental factors, and their interaction, in the etiology of melanoma. Three thousand, four hundred and seventy-one participants took part in the follow-up study and were administered a computer-assisted telephone interview in 2002-2005. Updated data on environmental and phenotypic risk factors, and 2777 blood samples were collected from interviewed participants as well as a subset of relatives. This study provides a large and well-described population-based sample of CMM cases with follow-up data. Characteristics of the cases and repeatability of sun exposure and phenotype measures between the baseline and the follow-up surveys, from 6 to 17 years later, are also described.