Double-mode radial-non-radial RR Lyrae stars. OGLE-IV photometry of two high cadence fields in the Galactic bulge

We analyse the OGLE-IV photometry of the first overtone and double-mode RR Lyrae stars (RRc/RRd) in the two fields towards the Galactic bulge observed with high cadence. In 27 per cent of RRc stars we find additional non-radial mode, with characteristic period ratio, P x /P 1O \in (0.6, 0.64). It strongly corroborates the conclusion arising from the analysis of space photometry of RRc stars, that this form of pulsation must be common. In the Petersen diagram the stars form three sequences. In 20 stars we find two or three close secondary modes simultaneously. The additional modes are clearly non-stationary. Their amplitude and/or phase vary in time. As a result, the patterns observed in the frequency spectra of these stars may be very complex. In some stars the additional modes split into doublets, triplets or appear as a more complex bands of increased power. Subharmonics of additional modes are detected in 20 per cent of stars. They also display a complex structure. Including our previous study of the OGLE-III Galactic bulge data, we have discovered 260 RRc and 2 RRd stars with the additional non-radial mode, which is the largest sample of these stars so far. The additional mode is also detected in two Blazhko RRc stars, which shows that the modulation and additional non-radial mode are not exclusive.Comment: 18 pages, 14 figures, accepted for publication in MNRA

Discovery of a new group of double-periodic RR Lyrae stars in the OGLE-IV photometry

We report the discovery of a new group of double-periodic RR Lyrae stars from the analysis of the OGLE-IV Galactic bulge photometry. In 11 stars identified in the OGLE catalog as first overtone pulsators (RRc stars) we detect additional longer period variability of low amplitude, in the mmag regime. One additional star of the same type is identified in a published analysis of the Kepler space photometry. The period ratio between the shorter first overtone period and a new, longer period lies in a narrow range around 0.686. Thus, the additional period is longer than the expected period of the undetected radial fundamental mode. The obvious conclusion that addition periodicity corresponds to a gravity or a mixed mode faces difficulties, however.Comment: 5 pages, 4 figures, accepted for publication in MNRAS Letter

OUTCOMES FOR YOUNG ADULTS IN EXTENDED FOSTER CARE

This study examined the outcomes for young adults in Extended Foster Care. Extended Foster Care is a relatively new program within the Child Welfare system, which provides services for former foster youth between the ages of 18 and 21 to become more successful, independent young adults. Before the implementation of Extended Foster Care in 2012, most of the foster children were left to fend for themselves after they turned 18, which resulted in negative outcomes. Extended Foster Care is a seemingly helpful program; however, due to its new existence there has been very limited research regarding the outcomes of these young adults in Extended Foster Care. This study used secondary data from the San Bernardino County Legislative, Research and Quality Support Services Unit. After data retrieval, independent t-tests and chi-squared tests were conducted using SPSS version 21. The independent variable of days spent in Extended Foster Care was compared to the following dependent variables: disability status, education status, housing status, and employment status and its barriers. The results of this study showed that the longer a young adults stays in Extended Foster Care, the higher their likelihood is of positive housing, employment, and education status. This study suggests it is critical to continue to provide Extended Foster Care services and further research needs to be conducted to ensure program quality and to continue to improve the services to this vulnerable, young adult population

Geochemical modelling of water-rock interaction

CO2 geological storage is one of the most promising technologies for reducing atmospheric emissions of greenhouse gas. In this work we present and discuss a new approach geochemical modelling for evaluating the effects of short-medium term CO2 disposal in deep geologic formations that has been tested in the Weyburn test site (Saskatchewan, Canada), where since September 2000 5000 t/day of supercritical CO2 are injected. The geochemical modeling has been performed by using the code PRHEEQC (V2.11) software package, via thermodynamic corrections to the code default database. First, we reconstructed the in-situ reservoir (62°C and 0.1 MPa) chemical composition, including pH, by the chemical equilibrium among the various phases, and we evaluated the boundary conditions (e.g. PCO2 , PH2S), which are necessary for the implementation of reaction path modeling. This is the starting point to assess the geochemical impact of CO2 into the oil reservoir and, as main target, to quantify water-gas-rock reactions. Furthermore, we identified possible compositions of the initially reservoir liquid phases by assuming the equilibrium conditions for the mineral assemblage with respect to a Na-Cl water (Cl/Na=1.2). Then we computed the kinetic evolution of the CO2-rich Weyburn brines interacting with the host-rock minerals, performed over 100 years after injection. Results of reaction path modeling suggest that, in this period, CO2 can be neutralized by solubility (as CO2 (aq)) and mineral trapping through Dawsonite precipitation. In order to validate our geochemical model we have simulated the geochemical impact of three years of CO2 injection (September 2000-2003) by kinetically controlled reactions and we have compared the computed and measured data. The calculated chemical composition after the CO2 injection is consistent with the analytical data of samples collected in 2003 with an error within 5 % for most analytical species, with the exception of the Ca and Mg contents (error > 90%), likely due to the complexation effect of carboxilic acid

Petersen Diagram Revolution

Over the recent years, the Petersen diagram for classical pulsators, Cepheids and RR Lyr stars, populated with a few hundreds of new multiperiodic variables. We review our analyses of the OGLE data, which resulted in the significant extension of the known, and in the discovery of a few new and distinct forms of multiperiodic pulsation. The showcase includes not only radial mode pulsators, but also radial-non-radial pulsators and stars with significant modulation observed on top of the beat pulsation. First theoretical models explaining the new forms of stellar variability are briefly discussed.Comment: 5 pages; to be published in the proceedings of the 22nd Los Alamos Stellar Pulsation Conference "Wide-field variability surveys: a 21st-century perspective", San Pedro de Atacama, Chile, Nov. 28 - Dec. 2, 201

Steuerbefreiung für Biokraftstoffe: Ist Bio-Ethanol wirklich eine klimapolitische Option?

In June 2002 the German Parliament decided to exempt biofuels from the gasoline tax. The policy to promote biofuels is being justified by allegedly positive effects on the climate, energy, and agricultural policy. The working paper takes a closer look at bio-ethanol as a substitute for gasoline and analyzes the underlying basic national and international conditions that provide the setting for the promotion of biofuels. Using energy and green house gas balances, the actual effects of the support and a possible increased use of biofuels are examined. The results show that the use of bio-ethanol to reduce green house gas emissions is economically inefficient and that there are other preferred alternative strategies.Im Juni 2002 hat der Deutsche Bundestag die Befreiung sämtlicher Biokraftstoffe von der Mineralölsteuer beschlossen. Eine solche Förderung von Biokraftstoffen wird von der Politik durch positive Effekte auf die Klima-, Energie- und Agrarpolitik gerechtfertigt. Das Arbeitspapier analysiert am Beispiel Bio-Ethanol als Benzinsubstitut auf nationaler und internationaler Ebene die Rahmenbedingungen, unter denen die Förderung stattfindet. Gleichzeitig werden anhand von Energie- und Treibhausgasbilanzen die tatsächlichen Auswirkungen der Förderung und einer möglichen vermehrten Verwendung von Bio-Ethanol untersucht. Dabei zeigt sich, dass die Verwendung von Bio-Ethanol zur Reduktion von Treibhausgasemissionen ineffizient ist und günstigere klimapolitische Alternativen zur Verfügung stehen

EPIC 201585823, a rare triple-mode RR Lyrae star discovered in K2 mission data

We have discovered a new, rare triple-mode RR Lyr star, EPIC 201585823, in the Kepler K2 mission Campaign 1 data. This star pulsates primarily in the fundamental and first-overtone radial modes, and, in addition, a third non-radial mode. The ratio of the period of the non-radial mode to that of the first-overtone radial mode, 0.616 285, is remarkably similar to that seen in 11 other triple-mode RR Lyr stars, and in 260 RRc stars observed in the Galactic bulge. This systematic character promises new constraints on RR Lyr star models. We detected subharmonics of the non-radial mode frequency, which are a signature of period doubling of this oscillation; we note that this phenomenon is ubiquitous in RRc and RRd stars observed from space, and from ground with sufficient precision. The non-radial mode and subharmonic frequencies are not constant in frequency or in amplitude. The amplitude spectrum of EPIC 201585823 is dominated by many combination frequencies among the three interacting pulsation mode frequencies. Inspection of the phase relationships of the combination frequencies in a phasor plot explains the ‘upward’ shape of the light curve. We also found that raw data with custom masks encompassing all pixels with significant signal for the star, but without correction for pointing changes, is best for frequency analysis of this star, and, by implication, other RR Lyr stars observed by the K2 mission. We compare several pipeline reductions of the K2 mission data for this star

Visual Multi-Metric Grouping of Eye-Tracking Data

We present an algorithmic and visual grouping of participants and eye-tracking metrics derived from recorded eye-tracking data. Our method utilizes two well-established visualization concepts. First, parallel coordinates are used to provide an overview of the used metrics, their interactions, and similarities, which helps select suitable metrics that describe characteristics of the eye-tracking data. Furthermore, parallel coordinates plots enable an analyst to test the effects of creating a combination of a subset of metrics resulting in a newly derived eye-tracking metric. Second, a similarity matrix visualization is used to visually represent the affine combination of metrics utilizing an algorithmic grouping of subjects that leads to distinct visual groups of similar behavior. To keep the diagrams of the matrix visualization simple and understandable, we visually encode our eye- tracking data into the cells of a similarity matrix of participants. The algorithmic grouping is performed with a clustering based on the affine combination of metrics, which is also the basis for the similarity value computation of the similarity matrix. To illustrate the usefulness of our visualization, we applied it to an eye-tracking data set involving the reading behavior of metro maps of up to 40 participants. Finally, we discuss limitations and scalability issues of the approach focusing on visual and perceptual issues