1,116 research outputs found

    PSB-045-Carpenter-Field Notes-1986

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    PSB CAT 203A-001-001 MANO

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    PSB CAT 106Z-010-001 MANO

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    PSB-Drawing-Op 106-Metate Fragments

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    PSB CAT 106Z-032-001-MANO

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    PSB CAT 106CC-011-001-MANO

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    Public priorities on locally-driven sea level rise planning on the East Coast of the United States

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    Sea level rise poses a substantial concern to communities worldwide. Increased inundation, storm surge, saltwater intrusion, and other impacts create challenges which will require considerable planning to address. Recognizing the broad and differing scope of sea level rise issues and the variability of policy options to address them, local planning frameworks are necessary in addition to tools and resources available from state and federal governments. To help assess priorities and preferences on sea level rise planning, a survey of 503 persons affiliated with coastal communities on the East Coast of the United States was conducted in December 2017. This survey studied key aspects locally-driven sea level rise plans, including planning priorities, funding options, methods to resolve conflict, and potential responses. Six key findings address these and other concerns to provide the foundation of a locally driven framework for public officials

    An ALMA Constraint on the GSC 6214-210 B Circum-Substellar Accretion Disk Mass

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    We present Atacama Large Millimeter/submillimeter Array (ALMA) observations of GSC 6214-210 A and B, a solar-mass member of the 5-10 Myr Upper Scorpius association with a 15 ±\pm 2 Mjup companion orbiting at ≈\approx330 AU (2.2"). Previous photometry and spectroscopy spanning 0.3-5 μ\mum revealed optical and thermal excess as well as strong Hα\alpha and Pa~β\beta emission originating from a circum-substellar accretion disk around GSC 6214-210 B, making it the lowest mass companion with unambiguous evidence of a subdisk. Despite ALMA's unprecedented sensitivity and angular resolution, neither component was detected in our 880 μ\mum (341 GHz) continuum observations down to a 3-σ\sigma limit of 0.22 mJy/beam. The corresponding constraints on the dust mass and total mass are <0.15 Mearth and <0.05 Mjup, respectively, or <0.003% and <0.3% of the mass of GSC 6214-210 B itself assuming a 100:1 gas-to-dust ratio and characteristic dust temperature of 10-20 K. If the host star possesses a putative circum-stellar disk then at most it is a meager 0.0015% of the primary mass, implying that giant planet formation has certainly ceased in this system. Considering these limits and its current accretion rate, GSC 6214-210 B appears to be at the end stages of assembly and is not expected to gain any appreciable mass over the next few Myr.Comment: Accepted to ApJ
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