17,697 research outputs found

    The essential signature of a massive starburst in a distant galaxy

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    Observations of carbon monoxide (CO) emission in high redshift (z>2) galaxies indicate the presence of large amounts of molecular gas. Many of these galaxies contain an active galactic nucleus (AGN) powered by accretion of gas onto a supermassive black hole, and a key question is whether their extremely high infrared luminosities result from the AGN, or from bursts of massive star formation (associated with the molecular gas), or both. In the Milky Way, high-mass stars form in the dense cores of interstellar molecular clouds; gas densities are n(H2)>105 cm-3 in the cores. Recent surveys show that virtually all galactic sites of high-mass star formation have similarly high densities. The bulk of the cloud material traced by CO observations is at a much lower density. In galaxies in the local Universe, the HCN(J=1-0) line is an effective tracer of the high-density molecular gas. Here we report observations of HCN emission in the early Universe from the infrared luminous 'Cloverleaf' quasar (at a redshift z=2.5579). The HCN line luminosity indicates the presence of 10 billion solar masses of very dense gas, an essential feature of an immense starburst that contributes, together with the AGN it harbors, to its high infrared luminosity.Comment: PDF pape

    MEVTV Workshop on Nature and Composition of Surface Units on Mars

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    Topics addressed include: SNC meteorites and their potential for providing information about the geochemical evolution of Mars; remote sensing; photogeological inferences of Martian surface compositions; and interactions of the surface with volatiles in either the surface or the atmosphere

    Monetary policy and economic activity: a postwar review

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    Monetary policy ; Financial markets ; Economic conditions

    Coherent pairing states for the Hubbard model

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    We consider the Hubbard model and its extensions on bipartite lattices. We define a dynamical group based on the η\eta-pairing operators introduced by C.N.Yang, and define coherent pairing states, which are combinations of eigenfunctions of η\eta-operators. These states permit exact calculations of numerous physical properties of the system, including energy, various fluctuations and correlation functions, including pairing ODLRO to all orders. This approach is complementary to BCS, in that these are superconducting coherent states associated with the exact model, although they are not eigenstates of the Hamiltonian.Comment: 5 pages, RevTe

    Space and surface power for the space exploration initiative: Results from project outreach

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    The analysis and evaluations of the Space and Surface Power panel, one of eight panels created by RAND to screen and analyze submissions to the Space Exploration Initiative (SEI) Outreach Program, is documented. In addition to managing and evaluating the responses, or submissions, to this public outreach program, RAND conducted its own analysis and evaluation relevent to SEI mission concepts, systems, and technologies. The Power panel screened and analyzed submissions for which a substantial portion of the concepts involved power generation sources, transmission, distribution, thermal management, and handling of power (including conditioning, conversion, packaging, and enhancements in system components). A background discussion of the areas the Power panel covered and the issues the reviewers considered pertinent to the analysis of power submissions are presented. An overview of each of the highest-ranked submissions and then a discussion of these submissions is presented. The results of the analysis is presented

    On the role of the weather in the deaths of R. F. Scott and his companions

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    A limit result for a system of particles in random environment

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    We consider an infinite system of particles in one dimension, each particle performs independant Sinai's random walk in random environment. Considering an instant tt, large enough, we prove a result in probability showing that the particles are trapped in the neighborhood of well defined points of the lattice depending on the random environment the time tt and the starting point of the particles.Comment: 11 page

    Mega-gifts in American Philanthropy: General & Jewish Giving Patterns Between 1995-2000

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    The researchers collected data on gifts of $10 million or above in order to compile this report. From this set, they identified gifts from Jewish philanthropists and offer some conclusions about the nature of high-end giving. Among other findings, the authors note that the largest number of gifts, by far, went to private educational institutions, and among Jewish donors, arts and culture was the second most popular recipient group. A listing of the donations is included in the appendices. With bibliographic references
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