On the use of rotational splitting asymmetries to probe the internal rotation profile of stars: Application to beta Cephei stars

Rotationally-split modes can provide valuable information about the internal rotation profile of stars. This has been used for years to infer the internal rotation behavior of the Sun. The present work discusses the potential additional information that rotationally splitting asymmetries may provide when studying the internal rotation profile of stars. We present here some preliminary results of a method, currently under development, which intends: 1) to understand the variation of the rotational splitting asymmetries in terms of physical processes acting on the angular momentum distribution in the stellar interior, and 2) how this information can be used to better constrain the internal rotation profile of the stars. The accomplishment of these two objectives should allow us to better use asteroseismology as a test-bench of the different theories describing the angular momentum distribution and evolution in the stellar interiors. (C) 2010 WILEY-VCH Verlag GmbH&Co. KGaA, Weinheim

VISTA Variables in the Via Lactea (VVV): The public ESO near-IR variability survey of the Milky Way

We describe the public ESO near-IR variability survey (VVV) scanning the Milky Way bulge and an adjacent section of the mid-plane where star formation activity is high. The survey will take 1929 h of observations with the 4-m VISTA telescope during 5 years (2010-2014), covering similar to 10(9) point sources across an area of 520 deg(2), including 33 known globular clusters and similar to 350 open clusters. The final product will be a deep near-IR atlas in five passbands (0.9-2.5 mu m) and a catalogue of more than 106 variable point sources. Unlike single-epoch surveys that, in most cases, only produce 2-D maps, the VVV variable star survey will enable the construction of a 3-D map of the surveyed region using well-understood distance indicators such as RR Lyrae stars, and Cepheids. It will yield important information on the ages of the populations. The observations will be combined with data from MACHO, OGLE, EROS, VST, Spitzer, HST, Chandra, INTEGRAL, WISE, Fermi LAT, XMM-Newton, GAIA and ALMA for a complete understanding of the variable sources in the inner Milky Way. This public survey will provide data available to the whole community and therefore will enable further studies of the history of the Milky Way, its globular cluster evolution, and the population census of the Galactic Bulge and center, as well as the investigations of the star forming regions in the disk. The combined variable star catalogues will have important implications for theoretical investigations of pulsation properties of stars. (C) 2009 Elsevier B.V. All rights reserved.

Chemical abundance analysis of the Be star HD 171054

In this work the results of a spectroscopic study of the southern field narrow-line Be star HD 171054 are presented. High dispersion and signal-to-noise ratio spectra allowed the estimation of the fundamental photospheric parameters such as the projected rotational velocity, effective temperature and superficial gravity from non-LTE stellar atmosphere models. From these parameters and microturbulence, the abundances of He, C, N, O, Mg, Al and Si for this object are estimated. Results show that C is depleted whereas N is overabundant compared with the sun and OB stars in the solar vicinity. Oxygen and helium are close to the solar value. Magnesium is down by 0.43 dex and aluminium and silicon are overabundant. (C) 2010 Elsevier B.V. All rights reserved.

Structural and spectroscopic characterization of poly(styrene sulfonate) films doped with neodymium ions

This work reports the structural and spectroscopy characterization of poly(styrene sulfonate) (PSS) films doped with neodymium (Nd) ions. Nd-PSS films were processed using the acid of poly(styrene sulfonate) - H-PSS and neodymium nitrate - Nd(NO(3))(3); the maximum incorporation of Nd ions in the polymeric matrix was equal 19.3%. The absorption in the UV-Vis-NIR spectral region presents typical electronic transitions of Nd 3, ions, with well resolved peaks. The infrared spectra present the transition bands of PSS with characteristic line shape broadening, and the presence of vibrational modes of N-O groups in the range of 1400-720 cm(-1), prove the permanence of Nd(NO(3))(x), with x = 1, 2 and/or 3. in the H-PSS matrix. UV-Vis site selective photoluminescence data indicate that the incorporation of Nd 31 introduces a blue shift in PSS emission (325-800 nm), decreasing the interaction between adjacent PSS lateral groups (aromatic rings). Nd(3+) reabsorption and energy transfer effects between the PSS matrix and Nd(3+) were also observed. The IR emission of Nd-PSS films at 1076 rim ((4)F(3/2) -> (4)I(11/2)) present constant efficiency, independent on Nd(3+) concentration. The Judd-Ofelt theory was employed to analyze radiative properties. The excitation spectra prove the energy transfer between the polymeric matrix and Nd(3+). Complex impedance data was used to probe relaxation processes during the charge transport within the polymeric matrix. (C) 2008 Elsevier B.V. All rights reserved.

Bayesian Estimation of the Logistic Positive Exponent IRT Model

A Bayesian inference approach using Markov Chain Monte Carlo (MCMC) is developed for the logistic positive exponent (LPE) model proposed by Samejima and for a new skewed Logistic Item Response Theory (IRT) model, named Reflection LPE model. Both models lead to asymmetric item characteristic curves (ICC) and can be appropriate because a symmetric ICC treats both correct and incorrect answers symmetrically, which results in a logical contradiction in ordering examinees on the ability scale. A data set corresponding to a mathematical test applied in Peruvian public schools is analyzed, where comparisons with other parametric IRT models also are conducted. Several model comparison criteria are discussed and implemented. The main conclusion is that the LPE and RLPE IRT models are easy to implement and seem to provide the best fit to the data set considered.

Can mass dissociation patterns of transition-metal complexes be predicted from electrochemical data?

The Cooks kinetic method has been very convenient to correlate the relative dissociation rates obtained by collision-induced fragmentation experiments with the energies of two related bonds in molecules and complexes in the gas phase. Reliable bond energy data are, however, not always available, particularly for polynuclear transition-metal complexes, such as the triruthenium acetate clusters of the general formula [Ru(3) (mu(3)-O)(mu-CH(3)COO)(6)(py)(2)(L)](+), where L = ring substituted N-heterocyclic ligands. Accordingly, their gas-phase collision-induced tandem mass spectrometry (CID MS/MS) dissociation patterns have been analyzed pursuing a relationship with the more easily accessible redox potentials (E(1/2)) and Lever`s E(L) parameters. In fact, excellent linear correlations of In(1/2A(L)/A(py)), where A(py) and A(L) are the abundance of the fragments retaining the pyridine (py) and L ligand, respectively, with E(1/2) and E(L) were found. This result shows that those electrochemical parameters are correlated with bond energies and can be used in the analysis of the dissociation data. Such modified Cooks method can be used, for example, to determine the electronic effects of substituents on the metal-ligand bonds for a series of transition-metal complexes. Copyright (C) 2008 John Wiley & Sons, Ltd.

Lithographic Technology Students in the Lab

Students are from the Lithography Department of the New York Trade School are shown working in a lab. Black and white photograph that has some writing along the outer edge.

Corridors for Wolf Reintroduction to Maine

Maine has been identified as holding potential for the reintroduction of wolves. Due to the long ranges of wolves, it is beneficial to map potential corridors of movement. This project analyzes the best routes for movement from suitable habitats in New York to suitable habitats in Maine. It shows the paths likely to be taken by wolves, based on their affinity for mixed and coniferous forest and their avoidance of areas of high road density. These corridors are identified using least cost path analysis and take into account topography as well as forest and road densities.

Alumni @ Large

Alumni notes Newsmakers Milestones Eyes and Ears: Jed Snyder '76 An Ounce of Prevention: Melissa Early Ruwitch '89 Beating the Odds: James Cryan '07 Obituaries

Type 8 Design B Port Side

print no 121, "1B.g. no 9." printed over "Blue Grey"; Discontinued stamp JUL 23 1918

Biorremediação de antraceno, fenantreno e pireno em um argissolo

O antraceno, o fenantreno e o pireno são hidrocarbonetos aromáticos policíclicos (HAPs) que podem ser carcinogênicos e que não são degradados pela maioria dos microrganismos do solo. A biorremediação é uma estratégia para eliminação dos HAPs, que pode demandar a inoculação de microrganismos degradadores e a modificação das condições químicas e físicas do solo. O objetivo do presente estudo foi isolar, identificar e caracterizar microrganismos degradadores e mineralizadores de antraceno, fenantreno e pireno em meio mineral e no solo, assim como avaliar a influência do pH e da disponibilidade de água, N, P, Fe e S na biorremediação de um solo contaminado com antraceno. Seis amostras de solo de landfarming foram inoculadas individualmente a um solo contaminado em laboratório com antraceno. Após 176 dias, o solo com maior produção de C-CO2 foi utilizado para o enriquecimento em meio mineral mais antraceno. Os microrganismos foram isolados e identificados pelo seqüenciamento do gene do RNAr. A capacidade dos microrganismos em degradar os 3 HAPs no meio mineral e no solo foi avaliada por cromatografia gasosa. A mineralização de diferentes concentrações de antraceno, fenantreno e pireno no solo foi avaliada por respirometria, assim como o efeito de diferentes doses de N, P, S e Fe, de diferentes pH e umidades do solo na mineralização do antraceno. Isolou-se do solo de landfarming um consórcio microbiano composto por 6 bactérias, identificadas como Mycobacterium fortuitum, Bacillus cereus, Microbacterium sp., Gordonia polyisoprenivorans, Microbacteriaceae bacterium e Naphthaleneutilizing bacterium, e um fungo, Fusarium oxysporum. O consórcio microbiano degradou respectivamente 48, 67 e 22% do antraceno, fenantreno e pireno do meio mineral. No solo o consórcio degradou, em média, mais de 92% e mineralizou mais de 78% das diferentes concentrações destes 3 HAPs em 70 dias. As maiores mineralizações do antraceno ocorreram nos solos com as maiores umidades gravimétricas (12,5%) e pH (7,5). A adição de 100 kg ha-1 ou mais de nitrogênio no solo e a conseqüente redução da relação C:N para valores inferiores a 67:1 diminuíram a mineralização do antraceno no solo. O aumento da disponibilidade do fósforo, do ferro e do enxofre e a presença de amplas relações C:P (1076:1 a 50:1) e C:N:P (1076:16:1 a 50:1,3:1) no solo não influenciaram a mineralização do antraceno. Conclui-se que a seleção e a inoculação ao solo de microrganismos degradadores de HAPs, associado a modificação das condições ambientais, pode conduzir a um eficiente processo de biorremediação, onde a grande maioria dos HAPs é mineralizada em curto período de tempo.