[Review of] William H. Turner and Edward J. Cabell, eds. Blacks in Appalachia

The editors are a civil rights worker (Cabell) and an academician (Turner) who evidence a longstanding interest in the Appalachian region and especially in the place and history of black people there. The articles are grouped into eight parts: Basic Approaches, Historical Perspectives, Community Studies, Race Relations, Black Coal Miners, Blacks and Local Politics, Personal Anecdotal Accounts of Black Life, and Selected Demographic Aspects. According to Turner\u27s article on the demography of Black Appalachia, he defines Appalachia as the Appalachian Regional Commission counties in Alabama, Georgia, Kentucky, North Carolina, South Carolina, Tennessee, Virginia and West Virginia

[Review of] Stephen Glazier, ed. Caribbean Ethnicity Re visited

Like marine life washed up on a beach, most Caribbean peoples have been brought where they are by powerful forces outside their control. These forces include colonialism, slavery, and revolution, processes in the seventeenth and eighteenth century that convulsed Europe and whose effects spread to much of the rest of the world. Just as tidepools a few feet apart can have completely different sets of animal and plant life, Caribbean islands just a few miles apart can have completely different histories and mixtures of peoples. Mirroring the complexity of the life in these tidepools, there are myriad interpretations of the effects of different historical, structural, cultural and other factors on the region. Stephen Glazier has selected a set of articles received from a call for papers placed in newsletters of the Caribbean Studies Association and the American Anthropological Association

Minimal surfaces in circle bundles over Riemann surfaces

For a compact 3-manifold $M$ which is a circle bundle over a compact Riemann surface $\Sigma$ with even Euler number $e(M)$, and with a Riemannian metric compatible with the bundle projection, there exists a compact minimal surface $S$ in $M$. $S$ is embedded and is a section of the restriction of the bundle to the complement of a finite number of points in $\Sigma$.Comment: 8 pages, no figures. Revised versio

Management of invasive Allee species

In this study, we use a discrete, two-patch population model of an Allee species to examine different methods in managing invasions. We first analytically examine the model to show the presence of the strong Allee effect, and then we numerically explore the model to test the effectiveness of different management strategies. As expected invasion is facilitated by lower Allee thresholds, greater carrying capacities and greater proportions of dispersers. These effects are interacting, however, and moderated by population growth rate. Using the gypsy moth as an example species, we demonstrate that the effectiveness of different invasion management strategies is context-dependent, combining complementary methods may be preferable, and the preferred strategy may differ geographically. Specifically, we find methods for restricting movement to be more effective in areas of contiguous habitat and high Allee thresholds, where methods involving mating disruptions and raising Allee thresholds are more effective in areas of high habitat fragmentation

Kepler's First Rocky Planet: Kepler-10b

NASA's Kepler Mission uses transit photometry to determine the frequency of Earth-size planets in or near the habitable zone of Sun-like stars. The mission reached a milestone toward meeting that goal: the discovery of its first rocky planet, Kepler-10b. Two distinct sets of transit events were detected: (1) a 152 ± 4 ppm dimming lasting 1.811 ± 0.024 hr with ephemeris T [BJD] = 2454964.57375^(+0.00060)_(–0.00082) + N * 0.837495^(+0.000004)_(–0.000005) days and (2) a 376 ± 9 ppm dimming lasting 6.86 ± 0.07 hr with ephemeris T [BJD] = 2454971.6761^(+0.0020)_(–0.0023) + N * 45.29485^(+0.00065) _(–0.00076) days. Statistical tests on the photometric and pixel flux time series established the viability of the planet candidates triggering ground-based follow-up observations. Forty precision Doppler measurements were used to confirm that the short-period transit event is due to a planetary companion. The parent star is bright enough for asteroseismic analysis. Photometry was collected at 1 minute cadence for >4 months from which we detected 19 distinct pulsation frequencies. Modeling the frequencies resulted in precise knowledge of the fundamental stellar properties. Kepler-10 is a relatively old (11.9 ± 4.5 Gyr) but otherwise Sun-like main-sequence star with T_(eff) = 5627 ± 44 K, M_⋆ = 0.895 ± 0.060 M_⊙ , and R_⋆ = 1.056 ± 0.021 R_⊙. Physical models simultaneously fit to the transit light curves and the precision Doppler measurements yielded tight constraints on the properties of Kepler-10b that speak to its rocky composition: M_P = 4.56^9+1.17)_(–1.29) M_⊕, R_P = 1.416^(+0.033)_(–0.036) R_⊕, and ρ_P = 8.8^(+2.1)_(–2.9) g cm^(–3). Kepler-10b is the smallest transiting exoplanet discovered to date

Higher homotopy operations and cohomology

We explain how higher homotopy operations, defined topologically, may be identified under mild assumptions with (the last of) the Dwyer-Kan-Smith cohomological obstructions to rectifying homotopy-commutative diagrams.Comment: 28 page