The Rondani Cecidomyiidae (Diptera)

The Rondani collection of Cecidomyiidae in Florence, Italy, is cataloged to account for existing specimens of Rondani species. Areport is made on the status and identity of each of Rondani's 16 species of Cecidomyiidae. Types of 12 species are represented by specimens in good to poor condition; those of the remaining four species cannot be found. Alectotypeis designated for Brachincura fuscogrisca and illustrations are given of its male genitalia and part of its antenna. Recommendations are made for future fixation of lectotypes or neotypes of some of Rondani's species

The gall midges (Diptera: Cecidomyiidae) of Acacia spp. (Mimosaceae) in Kenya

Twenty-eight new species of plant-feeding Cecidmnyiidae are described from galls taken on five species of Acacia in Kenya. The new species are placed in seven genera, four of them new. The new taxa, to be attributed to Gagne, are as follows, in bold face: in Acacidiplosis: ananas, cespitosa, conica, crispa, echinata, erupta, hamata, imbIicata, lamosa, lugosa, spinosa, undulata, and verticillata; in Aposchizomyia: acuta, brevis, crenata, longa, striata, and turnouri; Asphondylia napiformis; in Athidiplosis: bullata and walteri; in Contarinia. earolinae, hongoi, and plicata, Kimadiplosis divel sa, in Lupesia. niloticae and armata. The larvae, pupae, and the host-specific galls of these species generally offer the best characters for species discrimination. Galls of several additional species of gall midges from Acacia spp. in Kenya are described, but the gall makers are left unnamed for lack of suitable specimens. Collula acaciae (Kieffer 1912) is shown to be a junior homonym of Collula acaciae (Kieffer 1909) andis renamed kiefferi. Gail midges from acacias in Africa, India, and Australia are reviewed. Cecidomyia acaciaelongifoliae Skuse (1890) from Australia is newly combined in Dasineura. Two ofthe Bew species, Acacidiplodisspinosa and Aposehizomyia acula, inhibit flowering of Acacia nilotica and are potential biological control agents of their host in Australia

Ecología y diagnóstico de Enallodiplosis discordis (Diptera:Cecidomyiidae): Un nuevo defoliador feroz con repercusiones directas en la pérdida del bosque seco de Prosopis y los medios de vida en Perú

The coastal desert of Peru and Chile is home to Prosopis (Leguminosae: Mimosoideae) tree species that are exceptionally well-adapted to the hyperarid conditions and keystone in dry-forest ecosystems. From 2001 to 2018, Prosopis in Peru have suffered widespread defoliation and die-back, with consequent deforestation and collapse in pod production. This paper reports a new insect plague species of Prosopis forest in Peru: Enallodiplosis discordis Gagné 1994 (Diptera: Cecidomyiidae) as a fiercely defoliating agent contributing to widespread Prosopis mortality. An analysis of E. discordis larval taxonomy, life cycle and plague infestation, following El Niño Southern Oscillation (ENSO) 1998/99 is provided. Using distinct lines of evidence, its spread, distribution, and ecology are examined. Over two decades of fieldwork, Prosopis forest die-back and loss was observed devastating rural livelihoods and ecosystem services across lowland regions of southern (Ica), central and northern coastal Peru (Lambayeque, La Libertad, Piura). The collapse in production of Prosopis pods (algarroba, huaranga) and honey was recorded. Supplementary notes provide observations of: (i) plague development, changing land-use and climate, (ii) biological and physical control of E. discordis, (iii) the moth Melipotis aff. indomita (Lepidoptera: Noctuidae) as a concurrent defoliator of Prosopis.Las regiones desérticas costeras del Pacífico de Perú y Chile albergan especies de Prosopis (Leguminosae: Mimosoideae), árboles bien adaptados a las condiciones del desierto y con funciones clave en los ecosistemas de bosques secos. Entre el 2001 y 2017, Prosopis en Perú ha sufrido una extensiva defoliación y muerte regresiva, con la consecuente deforestación y disminución de la producción de vainas de algarrobo. Aquí, se reporta una nueva especie de insecto plaga del bosque de Prosopis en Perú: Enallodiplosis discordis Gagné 1994 (Diptera: Cecidomyiidae), una feroz especie defoliadora que contribuye a la mortalidad generalizada de Prosopis. Se proporciona un análisis de la taxonomía larvaria de E. discordis, ciclo de vida y la infestación ocurrida después de El Niño Oscilación del Sur (ENSO) 1998/99. Su dispersión, distribución y ecología es examinada utilizando distintas líneas de evidencia. Durante casi dos décadas de trabajo de campo, se observó la muerte regresiva del bosque de Prosopis devastando los medios de vida rurales y los servicios de los ecosistemas en las regiones de las tierras bajas del sur (Ica), el centro y el norte de la costa peruana (Lambayeque, La Libertad, Piura). El colapso en la producción de vainas de Prosopis (algarroba, huaranga) y miel también fue registrada. Las notas complementarias proporcionan observaciones sobre: (i) el desarrollo de la plaga y el cambio de uso de la tierra y el clima, (ii) el control biológico y físico de E. discordis, (iii) la polilla Melipotis aff. indomita (Lepidoptera: Noctuidae) como defoliador concurrente de Prosopis

A Deep Chandra X-ray Spectrum of the Accreting Young Star TW Hydrae

We present X-ray spectral analysis of the accreting young star TW Hydrae from a 489 ks observation using the Chandra High Energy Transmission Grating. The spectrum provides a rich set of diagnostics for electron temperature T_e, electron density N_e, hydrogen column density N_H, relative elemental abundances and velocities and reveals its source in 3 distinct regions of the stellar atmosphere: the stellar corona, the accretion shock, and a very large extended volume of warm postshock plasma. The presence of Mg XII, Si XIII, and Si XIV emission lines in the spectrum requires coronal structures at ~10 MK. Lower temperature lines (e.g., from O VIII, Ne IX, and Mg XI) formed at 2.5 MK appear more consistent with emission from an accretion shock. He-like Ne IX line ratio diagnostics indicate that T_e = 2.50 +/- 0.25 MK and N_e = 3.0 +/- 0.2 x 10^(12) cm^(-3) in the shock. These values agree well with standard magnetic accretion models. However, the Chandra observations significantly diverge from current model predictions for the postshock plasma. This gas is expected to cool radiatively, producing O VII as it flows into an increasingly dense stellar atmosphere. Surprisingly, O VII indicates N_e = 5.7 ^(+4.4}_(-1.2) x 10^(11) cm^(-3), five times lower than N_e in the accretion shock itself, and ~7 times lower than the model prediction. We estimate that the postshock region producing O VII has roughly 300 times larger volume, and 30 times more emitting mass than the shock itself. Apparently, the shocked plasma heats the surrounding stellar atmosphere to soft X-ray emitting temperatures and supplies this material to nearby large magnetic structures -- which may be closed magnetic loops or open magnetic field leading to mass outflow. (Abridged)Comment: 13 pages (emulateapj style), 10 figures, ApJ, in pres

Description of the Larva of Lophodiplosis trifida, an Australian Gall Midge (Diptera: Cecidomyiidae) and Biocontrol Agent of Paperbark in

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Unveiling the Cygnus OB2 stellar population with Chandra

The aim of this work is to identify the so far unknown low mass stellar population of the ~2Myr old Cygnus OB2 region, and to investigate the X-ray and near-IR stellar properties of its members. We analyzed a 97.7 ksec Chandra ACIS-I observation pointed at the core of the Cygnus OB2 region. X-ray variability ans spectral analysis of sources was characterized through the KS-test and XSPEC thermal models, respectively. We detected 1003 X-ray sources. Of these, 775 have near-IR counterparts associated with Cygnus OB2 members. We estimate a typical absorption toward Cygnus OB2 of Av~7.0 mag. Although the region is young, very few stars (~4.4 %) show disk-induced excesses in the near-IR. X-ray variability is detected in ~13 % of the sources. Flares account for at least 60 % of the variability. O- that early B-type stars are not significantly variable. Typical X-ray spectral parameters are log(Nh)~22.25 and kT~1.35 keV. Variable and flaring sources have harder spectra with median kT=3.3 and 3.8 keV, respectively. OB stars are typically softer (kT~0.75 keV). X-ray luminosities range between 1E+30 and 1E+31 erg/s for intermediate- and low-mass stars, and 2.5x10^30 and between 6.3E+33 erg/s for OB stars. The Cygnus OB2 region has a very rich population of low-mass X-ray emitting stars. Circumstellar disks seem to be very scarce.Comment: Accepted for publication in A&A. 20 pages, 17 figure

XMM-Newton X-ray study of early type stars in the Carina OB1 association

<p><b>Aims:</b> X-ray properties of the stellar population in the Carina OB1 association are examined with special emphasis on early-type stars. Their spectral characteristics provide some clues to understanding the nature of X-ray formation mechanisms in the winds of single and binary early-type stars.</p> <p><b>Methods:</b> A timing and spectral analysis of five observations with XMM-Newton is performed using various statistical tests and thermal spectral models.</p> <p><b>Results:</b> 235 point sources have been detected within the field of view. Several of these sources are probably pre-main sequence stars with characteristic short-term variability. Seven sources are possible background AGNs. Spectral analysis of twenty four sources of type OB and WR 25 was performed. We derived spectral parameters of the sources and their fluxes in three energy bands. Estimating the interstellar absorption for every source and the distance to the nebula, we derived X-ray luminosities of these stars and compared them to their bolometric luminosities. We discuss possible reasons for the fact that, on average, the observed X-ray properties of binary and single early type stars are not very different, and give several possible explanations.</p&gt

Untangling knowledge creation and knowledge integration in enterprise wikis

A central challenge organizations face is how to build, store, and maintain knowledge over time. Enterprise wikis are community-based knowledge systems situated in an organizational context. These systems have the potential to play an important role in managing knowledge within organizations, but the motivating factors that drive individuals to contribute their knowledge to these systems is not very well understood. We theorize that enterprise wiki initiatives require two separate and distinct types of knowledge-sharing behaviors to succeed: knowledge creation (KC) and knowledge integration (KI). We examine a Wiki initiative at a major German bank to untangle the motivating factors behind KC and KI. Our results suggest KC and KI are indeed two distinct behaviors, reconcile inconsistent findings from past studies on the role of motivational factors for knowledge sharing to establish shared electronic knowledge resources in organizations, and identify factors that can be leveraged to tilt behaviors in favor of KC or KI

Four new genera of Nearctic Cecidomyiidae (Diptera) for species previously incorrectly placed

Gagné, Raymond J. (2013): Four new genera of Nearctic Cecidomyiidae (Diptera) for species previously incorrectly placed. Zootaxa 3701 (2): 148-158, DOI: 10.11646/zootaxa.3701.2.

Key to Adults of North American Genera of the Subfamily Cecidomyiinae (Diptera: Cecidomyiidae)

Gagné, Raymond J. (2018): Key to Adults of North American Genera of the Subfamily Cecidomyiinae (Diptera: Cecidomyiidae). Zootaxa 4392 (3): 401-457, DOI: https://doi.org/10.11646/zootaxa.4392.3.