27 research outputs found

    Catching Element Formation In The Act

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    Gamma-ray astronomy explores the most energetic photons in nature to address some of the most pressing puzzles in contemporary astrophysics. It encompasses a wide range of objects and phenomena: stars, supernovae, novae, neutron stars, stellar-mass black holes, nucleosynthesis, the interstellar medium, cosmic rays and relativistic-particle acceleration, and the evolution of galaxies. MeV gamma-rays provide a unique probe of nuclear processes in astronomy, directly measuring radioactive decay, nuclear de-excitation, and positron annihilation. The substantial information carried by gamma-ray photons allows us to see deeper into these objects, the bulk of the power is often emitted at gamma-ray energies, and radioactivity provides a natural physical clock that adds unique information. New science will be driven by time-domain population studies at gamma-ray energies. This science is enabled by next-generation gamma-ray instruments with one to two orders of magnitude better sensitivity, larger sky coverage, and faster cadence than all previous gamma-ray instruments. This transformative capability permits: (a) the accurate identification of the gamma-ray emitting objects and correlations with observations taken at other wavelengths and with other messengers; (b) construction of new gamma-ray maps of the Milky Way and other nearby galaxies where extended regions are distinguished from point sources; and (c) considerable serendipitous science of scarce events -- nearby neutron star mergers, for example. Advances in technology push the performance of new gamma-ray instruments to address a wide set of astrophysical questions.Comment: 14 pages including 3 figure

    Grazing and light modify Silene latifolia responses to nutrients and future climate

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    Altered climate, nutrient enrichment and changes in grazing patterns are important environmental and biotic changes in temperate grassland systems. Singly and in concert these factors can influence plant performance and traits, with consequences for species competitive ability, and thus for species coexistence, community composition and diversity. However, we lack experimental tests of the mechanisms, such as competition for light, driving plant performance and traits under nutrient enrichment, grazer exclusion and future climate. We used transplants of Silene latifolia, a widespread grassland forb in Europe, to study plant responses to interactions among climate, nutrients, grazing and light. We recorded transplant biomass, height, specific leaf area (SLA) and foliar carbon to nitrogen ratio (C:N) in full-factorial combinations of future climate treatment, fertilization, grazer exclusion and light addition via LED-lamps. Future climate and fertilization together increased transplant height but only in unlighted plots. Light addition increased SLA in ambient climate, and decreased C:N in unfertilized plots. Further, transplants had higher biomass in future climatic conditions when protected from grazers. In general, grazing had a strong negative effect on all measured variables regardless of added nutrients and light. Our results show that competition for light may lead to taller individuals and interacts with climate and nutrients to affect traits related to resource-use. Furthermore, our study suggests grazing may counteract the benefits of future climate on the biomass of species such as Silene latifolia. Consequently, grazers and light may be important modulators of individual plant performance and traits under nutrient enrichment and future climatic conditions

    Regression of <i>Silene</i> height and vegetation and litter cover.

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    Regression of the visually estimated (a) total vegetation cover and Silene height and (b) litter cover and Silene height. The line represents a regression line with a 95% CI. The regressions are significant (a) F1,74 = 7.58, P = 0.007 (b) F1,56 = 21.74, P (TIF)</p

    Treatment effects on <i>Silene</i> performance.

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    Height (a, n = 80) and biomass (b, n = 78) responses of Silene latifolia to combinations of grazing, fertilization, ambient and future climate and light addition. The data are means ± SE. Note, that two transplants were not harvested for biomass determination because they were grazed to a few millimeters from the ground.</p

    Main and interactive treatment effects on <i>Silene</i> performance.

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    Main and interactive treatment effects on Silene performance.</p

    Main and interactive treatment effects on <i>Silene</i> foliar traits.

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    Main and interactive treatment effects on Silene foliar traits.</p

    Treatment effects on <i>Silene</i> foliar traits.

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    Foliar C:N (a, n = 36) and SLA (b, n = 32) responses of Silene latifolia to combinations of fertilization, ambient and future climate and light addition. The data are from inside the fences and represent means ± SE. Note, that there are less than 40 samples per trait, because some transplants did not have healthy and undamaged leaves.</p

    Treatment effects on vegetation and litter cover.

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    (a) Percent total vegetation cover and (b) percent litter cover in grazed (sheep) and ungrazed (exclosure), unfertilized and fertilized plots under ambient and future climate conditions. Data are means ± SE. Total vegetation cover and litter cover were assessed by visual estimation on the experimental plots in June 2020. (TIF)</p

    Regression of <i>Silene</i> SLA and light intensity and litter cover.

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    Regression of (a) the light intensity measured approximately 7–10 cm under the lamps and 15–20 cm above ground level and Silene SLA and (b) the visually estimated percentage litter cover and Silene SLA. The lines represent regression lines with a 95% CI. The dashed regression line is not significant (F1,29 = 0.38, P = 0.544), the solid regression line is significant (F1,44 = 13.67, P (TIF)</p
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