10,375 research outputs found

    Notes on the Life cycle of \u3ci\u3eNemoria Rubrifrontaria\u3c/i\u3e (Lepidoptera: Geometridae)

    Get PDF
    (excerpt) While surveying for insect pests of sweet fern, Myrica aspleniifolia L., two unidentified eggs were detected on foliage samples collected in June 1972 near Barton City, Alcona County, Michigan. the eggs were transferred to petri dishes with sweet fern foliage for rearing. Subsequently, one of the larvae that emerged was reared to adulthood and identified as Nemoria rubrifrontaria Packard. This note describes the life cycle of this insect

    Life History, Damage, and Gall Development of the Gall Midge, \u3ci\u3eNeolasioptera Brevis\u3c/i\u3e (Diptera: Cecidomyiidae), Injurious to Honeylocust in Michigan

    Get PDF
    Neolasioptera brevis is univoltine in Michigan. Adults issue in late spring, and females deposit eggs in rows on the lower side of young shoots of honeylocust. Larval eclosion occurs shortly after: there are three larval instars. The gall is polythalamous and may have 20 or more larvae. The third-instar larvae overwinter, and pupation occurs in spring. The gall injury kills sorne shoots, but most damage is cosmetic. One can monitor for adult emergence in late April or May by observing cast pupal cases protruding from the gall. Control, if needed, should be directed at adults

    Extreme CO Isotopic Abundances in the ULIRG IRAS 13120-5453: An Extremely Young Starburst or Top-Heavy Initial Mass Function

    Get PDF
    We present ALMA 12^{12}CO (J=1-0, 3-2 and 6-5), 13^{13}CO (J=1-0) and C18^{18}O (J=1-0) observations of the local Ultra Luminous Infrared Galaxy, IRAS 13120-5453 (dubbed "The Yo-yo"). The morphologies of the three isotopic species differ, where 13^{13}CO shows a hole in emission towards the center. We measure integrated brightness temperature line ratios of 12^{12}CO/13^{13}CO ≥\geq 60 (exceeding 200) and 13^{13}CO/C18^{18}O ≤\leq 1 in the central region. Assuming optical thin emission, C18^{18}O is more abundant than 13^{13}CO in several regions. The abundances within the central 500 pc are consistent with enrichment of the ISM via a young starburst (<<7Myr), a top-heavy initial mass function or a combination of both.Comment: 7 pages, 3 figures, accepted for publication in ApJ

    Review Essay—Battle on the Potomac

    Get PDF
    This War Really Matters: Inside the Fight for Defense Dollar

    Analysis of the temporal electric fields in lossy dielectric media

    Get PDF

    Influence of bulk dielectric polarization and void geometry upon PD transients

    Get PDF
    • …
    corecore