Dark Matter in the Milky Way's Dwarf Spheroidal Satellites

The Milky Way's dwarf spheroidal satellites include the nearest, smallest and least luminous galaxies known. They also exhibit the largest discrepancies between dynamical and luminous masses. This article reviews the development of empirical constraints on the structure and kinematics of dSph stellar populations and discusses how this phenomenology translates into constraints on the amount and distribution of dark matter within dSphs. Some implications for cosmology and the particle nature of dark matter are discussed, and some topics/questions for future study are identified.Comment: A version with full-resolution figures is available at http://www.cfa.harvard.edu/~mwalker/mwdsph_review.pdf; 70 pages, 22 figures; invited review article to be published in Vol. 5 of the book "Planets, Stars, and Stellar Systems", published by Springe

Proteomic analysis of the reproductive tract fluids from tropically-adapted Santa Ines rams

Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)The present study is focused on the proteome of reproductive tract fluids from tropically-adapted Santa Ines rams. Seminal plasma, cauda epididymal (CEF) and vesicular gland fluid (VGF) proteins were analyzed by 2-D electrophoresis and mass spectrometry. Seminal plasma maps contained 302 +/- 16 spots, within the 4-7 pH range. From these maps, 73 spots were identified, corresponding to 41 proteins. Ram Seminal Vesicle Proteins (RSVP) 14 and 22 kDa and bodhesins 1 and 2 represented the most abundant seminal components. Other seminal proteins included clusterin, angiotensin-converting enzyme, matrix metalloproteinase-2, tissue-inhibitor of metalloproteinase-2, plasma glutamate carboxypeptidase, albumin, lactoferrin, alpha enolase, peroxiredoxin, leucine aminopeptidase, beta-galactosidase, among others. Later, seminal plasma gels were run within narrow pH intervals (3.9-5.1; 4.7-5.9; 5.5-6.7), allowing the additional identification of 21 proteins not detected in 4-7 pH maps. Major proteins of CEF and VGF were albumin and transferrin, and RSVPs, respectively. Western blots confirmed that RSVPs were mainly present in VGF while bodhesins, in VGF and CEF. Based on RT-PCR, RSVP and bodhesin genes were primarily expressed in the vesicular glands. In summary, the reproductive tract fluids of Brazilian hairy rams contain several categories of proteins, with potential roles in sperm protection, capacitation, acrosome reaction and sperm-oocyte interaction. This article is part of a Special Issue entitled: Farm animal proteomics. (c) 2012 Elsevier B.V. All rights reserved.7514SI44364456Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)Ceara State Research Foundation (FUNCAP)Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES