Europe: So Many Languages, So Many Cultures

The number of different languages in Europe by far exceeds the number of countries. All European countries have national languages, and in nearly all of them there are minority languages as well, whereas all major languages have dialects. National borders rarely coincide with linguistic borders, but the latter (including dialect borders) mark by their nature also more or less distinct cultural areas. This paper presents a survey of the different language families represented in Europe: Indo-European, Uralic, Altaic, and the four Caucasian language families, each with their sub-branches and individual languages. Some information is given on characteristic structural phenomena and on the status and history of these languages or language families and on some of their extinct predecessors. The paper ends with a short discussion on the language policy and practices of the institutions of the European Union. Europe lacks a language with the status and power comparable to Indonesian in Indonesia. The policy is therefore based on equal status of all national languages and on respect for all languages, including national minority ones. The practice, however, is unavoidably practical: “the more languages, the more English”

Tolerance to Hairy Chinch Bug Feeding in Kentucky Bluegrass

Seventeen Kentucky bluegrass, Poa pratensis L., cultivars were evaluated for tolerance to feeding by adult hairy chinch bugs, Blissus leucopterus hirtus Montandon. Adults were confined on one month-old plants within a 10 cm diam × 20.3 cm high cylindrical plastic cage for 17-19 days. Cages were divided longitudinally so that 1/2 of the plants in each pot were infested. Tolerance was evaluated as differences between infested and uninfested plants for height of regrowth, dry weight, yield of clippings, root length and weight, plant survival, tillering, and % dry matter. Regrowth, yield of clippings, root length, and plant survival were significantly reduced and % dry matter significantly increased in almost all cases by adult feeding. Dry weight, root weight, and tillering of plants were not significantly changed by feeding. Significant differences were found in tolerance among Kentucky bluegrass cultivars. Differences in cultivar regrowth, yield, and % dry matter were the most useful criteria for measuring toleranc

Laboratory Rearing of the Hairy Chinch Bug

Laboratory procedures were developed for rearing the hairy chinch bug Blissus leucopterus hirtus Montandon, on corn sections in 236.6 ml cardboard cartons. There was significantly higher survival of nymphs and adults when eggs were surface sterilized in 2% sodium hypochlorite solution as compared to those treated with a 1% solution or untreated eggs. Adult survival was significantly higher (P<0.05) when chinch bugs were reared on corn sections treated with 2% sodium hypochlorite than when either treated with 2% thiram or untreated. Developmental times for nymphal instars were determined as follows: 1st 12.3±6.0; 2nd 5.4±2.7; 3rd 5.2±1.7; 4th 4.9±1.3; 5th 7.1±0.9; total 35.5±7.4 days. The preoviposition period was determined to be 1O.8±4.4 days with nearly 80% of the females tested ovipositing within 24 day

WIYN Open Cluster Study XI: WIYN 3.5m Deep Photometry of M35 (NGC 2168)

We present deep BVI observations of the core of M35 and a nearby comparison field obtained at the WIYN 3.5m telescope under excellent seeing. These observations display the lower main sequence in BV and VI CMDs down to V = 23.3 and 24.6, respectively. At these faint magnitudes background field stars are far more numerous than the cluster stars, yet by using a smoothing technique and CMD density distribution subtraction we recover the cluster fiducial main sequence and luminosity function to V = 24.6. We find the location of the main sequence in these CMDs to be consistent with earlier work on other open clusters, specifically NGC 188, NGC 2420, and NGC 2477. We compare these open cluster fiducial sequences to stellar models by Baraffe et al. (1998), Siess et al. (2000), Girardi et al. (2000), and Yi et al. (2001) and find that the models are too blue in both B-V and V-I for stars below ~0.4 Mo. M35 contains stars to the limit of the extracted main sequence, at M ~ 0.10-0.15 Mo, suggesting that M35 may harbor a large number of brown dwarfs, which should be easy targets for near-IR instrumentation on 8-10m telescopes. We also identify a new candidate white dwarf in M35 at V = 21.36 +- 0.01. Depending on which WD models are used to interpret this cluster candidate, it is either a very high mass WD (1.05 +- 0.05 Mo) somewhat older (0.19-0.26 Gyr, 3-4 sigma) than our best isochrone age (150 Myr), or it is a modestly massive WD (0.67-0.78 Mo) much too old (0.42-0.83 Gyr) to belong to the cluster.Comment: 28 pages + 24 figures; to be published in the Sept, 2002 A

Perfluoro Alkyl Hypofluorites and Peroxides Revisited

A more convenient synthesis of the perfluoro alkyl hypofluorite (F3C)3COF as well as the hitherto unknown (C2F5)(F3C)2COF compound is reported. Both hypofluorites can be prepared by use of the corresponding tertiary alcohols RFOH and elemental fluorine in the presence of CsF. An appropriate access to these highly reactive hypofluorites is crucial. The hypofluorites are then transferred into their corresponding perfluoro bisalkyl peroxides RFOORF [RF=(F3C)3C, (C2F5)(F3C)2C] by treatment with partially fluorinated silver wool. NMR, gas‐phase infrared, and solid‐state Raman spectra of the perfluoro bisalkyl peroxides are presented and their chemical properties are discussed