276 research outputs found

    Apparatus automatically measures soluble residue content of volatile solvents

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    Solvent Purity Meter /SPM/ automatically measures the soluble residue in volatile solvents used in cleaning or extraction of oils, greases, and other nonvolatile materials. The SPM gives instantaneous and continuous readout of soluble contaminant residues in concentrations as low as one part per million of solution

    Public Access to the Beaches of Connecticut

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    Elements of the public of Connecticut are engaged in direct conflict against private and municipal property rights over the issue of increased public access to beaches of the state. In Connecticut, as well as the nation, definite solutions to the problem are slow to materialize. The public\u27s right to the whole beach is being clarified by only a few states, while public access under common law remains a clouded issue nationwide. The research study I am proposing would examine in detail the legal issues involved, the state and federal legislative actions, geographical considerations, etc. I feel that the resulting collation of the issues and alternative solutions will assist the state planners and decision makers of Connecticut in resolving the problem of public access to the beaches of Connecticut

    Grain Sorghum Performance Trials

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    Book Reviews

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    Book Reviews

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    UV Observations of the Cool DBQA5 White Dwarf LDS 678A - Limits on the Atmospheric Composition, Pressure Shift, and Gravitational Redshift Derived from C I 2479

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    A high-resolution ultraviolet spectrum of the helium-rich degenerate LDS 678A, obtained with the International Ultraviolet Explorer (IUE) satellite, is presented. LDS 678A is the coolest metallic line degenerate (DQ or DZ) yet observed with the IUE echelle. These observations provide a detailed line profile of the strong C I 2479 absorption line and equivalent width W2479 = 2.35 + or - 0.06 A from which theoretical profile fits yield a carbon abundance of log C/He = (-6.7 + or- 0.2). The presence of carbon in a He-rich atmosphere lends credence to the notion that LDS 678A is a transitional case between the DB white dwarfs with nearly pure helium atmospheres and the helium-rich DQ white dwarfs which exhibit carbon bands. Corrected for an inferred pressure shift Vp = + 38 + or - 4 km/s for the C I 2479 line, a gravitational redshift of Vrs = + 26 + or - 13 km/s is deduced from which a most probable mass of 0.55 solar mass is derived

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    Where Are the Magnetic White Dwarfs with Detached, Nondegenerate Companions?

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    The Sloan Digital Sky Survey has already more than doubled the sample of white dwarfs with spectral classifications, the subset with detached M dwarf companions, and the subset of magnetic white dwarfs. In the course of assessing these new discoveries, we have noticed a curious, unexpected property of the total lists of magnetic white dwarfs and of white dwarf plus main-sequence binaries: there appears to be virtually zero overlap between the two samples! No confirmed magnetic white dwarf has yet been found in such a pairing with a main-sequence star. The same statement can be made for the samples of white dwarf–M dwarf pairs in wide, common proper motion systems. This contrasts with the situation for interacting binaries, in which an estimated 25% of the accreting systems have a magnetic white dwarf primary. Alternative explanations are discussed for the observed absence of magnetic white dwarf–main-sequence pairs, but the recent discoveries of very low accretion rate magnetic binaries pose difficulties for each. A plausible explanation may be that the presence of the companion and the likely large mass and small radius of the magnetic white dwarf (relative to nonmagnetic degenerate dwarfs) may provide a selection effect against the discovery of the latter in such binary systems. More careful analysis of the existing samples may yet uncover members of this class of binary, and the sample sizes will continue to grow. The question of whether the mass and field distributions of the magnetic primaries in interacting binaries are similar to those of the isolated magnetic white dwarfs (including those in wider binaries) must also be answered

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