Sexual Size Dimorphism, Ovipositioning, and Hatching in Leiocephalus macropus asbolomus (Squamata: Leiocephalidae) in Alexander von Humboldt National Park in Eastern Cuba

The endemic Antillean family Leiocephalidae includes 28 currently recognized extant species in the genus Leiocephalus. These are distributed across Hispaniola, Cuba, and various islands and cays in the Bahamas. Sexual size dimorphism (SSD)  is a fundamental and widespread biological phenomenon generally attributed to sexual differences  in relationships between body size, survival, fecunditty, and mating success. Six species with 40 subspecies are known from Cuba. Few data are available regarding SSD and reproduction. Herein we report new life-history data and the sexual size dimorphism index (SSDI) in Leiocephalus macropus asbolomus. Fieldwork was performed  during mid-August 2009 iin La Melba (Alexander von Humboldt National Park), HolguinProvince, Cuba. All males were larger in size then females and the SSDI (1.44) is the highest reported ffor any species of Leiocephalus. Egg measurments averaged 18.2 x 12.7 mml mean clutch size was 3. Eggs took 61-72 days to hatch; mean incubation time was 66.5 days, and mean hatchling SVL was 30.1 mm. &nbsp

'BRS Magna': nova cultivar de uva para suco com ampla adaptação climática.

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'BRS Vitória': a novel seedless table grape cultivar exhibiting special flavor and tolerance to downy mildew (Pasmopara viticola).

'BRS Vitória' is a novel cultivar of black seedless table grape. Its main traits meet the most important demands from the viticulture segment in Brazil. It is recommended for cultivation in tropical and subtropical areas, with excellent horticultural performance, high bud fecundity and resistance to downy mildew, the most important disease which affects grapevines in Brazil.Cultivar release

'BRS Vitória': nova cultivar de uva de mesa sem sementes com sabor especial e tolerante ao míldio.

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Structure and Colors of Diffuse Emission in the Spitzer Galactic First Look Survey

We investigate the density structure of the interstellar medium using new high-resolution maps of the 8 micron, 24 micron, and 70 micron surface brightness towards a molecular cloud in the Gum Nebula, made as part of the Spitzer Space Telescope Galactic First Look Survey. The maps are correlated with 100 micron images measured with IRAS. At 24 and 70 micron, the spatial power spectrum of surface brightness follows a power law with spectral index -3.5. At 24 micron, the power law behavior is remarkably consistent from the 0.2 degree size of our maps down to the 5 arcsecond spatial resolution. Thus, the structure of the 24 micron emission is self-similar even at milliparsec scales. The combined power spectrum produced from Spitzer 24 micron and IRAS 25 micron images is consistent with a change in the power law exponent from -2.6 to -3.5. The decrease may be due to the transition from a two-dimensional to three-dimensional structure. Under this hypothesis, we estimate the thickness of the emitting medium to be 0.3 pc.Comment: 13 Pages, 3 Figures, to be published in Astrophysical Journal Supplement Series (Spitzer Special Issue), volume 154. Uses aastex v5.

Observations of Ultraluminous Infrared Galaxies with the Infrared Spectrograph on the Spitzer Space Telescope: Early Results on Mrk 1014, Mrk 463, and UGC 5101

We present spectra taken with the Infrared Spectrograph on Spitzer covering the 5-38micron region of three Ultraluminous Infrared Galaxies (ULIRGs): Mrk 1014 (z=0.163), and Mrk 463 (z=0.051), and UGC 5101 (z=0.039). The continua of UGC 5101 and Mrk 463 show strong silicate absorption suggesting significant optical depths to the nuclei at 10microns. UGC 5101 also shows the clear presence of water ice in absorption. PAH emission features are seen in both Mrk 1014 and UGC 5101, including the 16.4micron line in UGC 5101. The fine structure lines are consistent with dominant AGN power sources in both Mrk 1014 and Mrk 463. In UGC 5101 we detect the [NeV] 14.3micron emission line providing the first direct evidence for a buried AGN in the mid-infrared. The detection of the 9.66micron and 17.03micron H$_{2}$ emission lines in both UGC 5101 and Mrk 463 suggest that the warm molecular gas accounts for 22% and 48% of the total molecular gas masses in these galaxies.Comment: Accepted in ApJ Sup. Spitzer Special Issue, 4 pages, 3 figure