916 research outputs found
The history of stellar metallicity in a simulated disc galaxy
We explore the chemical distribution of stars in a simulated galaxy. Using simulations of the same initial conditions but with two different feedback schemes (McMaster Unbiased Galaxy Simulations â MUGS â and Making Galaxies in a Cosmological Context â MaGICC), we examine the features of the ageâmetallicity relation (AMR), and the three-dimensional ageâ [Fe/H]â[O/Fe] distribution, both for the galaxy as a whole and decomposed into disc, bulge, halo and satellites. The MUGS simulation, which uses traditional supernova feedback, is replete with chemical substructure. This substructure is absent from the MaGICC simulation, which includes early feedback from stellar winds, a modified initial mass function and more efficient feedback. The reduced amount of substructure is due to the almost complete lack of satellites in MaGICC. We identify a significant separation between the bulge and disc AMRs, where the bulge is considerably more metal-rich with a smaller spread in metallicity at any given time than the disc. Our results suggest, however, that identifying the substructure in observations will require exquisite age resolution, of the order of 0.25 Gyr. Certain satellites show exotic features in the AMR, even forming a âsawtoothâ shape of increasing metallicity followed by sharp declines which correspond to pericentric passages. This fact, along with the large spread in stellar age at a given metallicity, compromises the use of metallicity as an age indicator, although alpha abundance provides a more robust clock at early times. This may also impact algorithms that are used to reconstruct star formation histories from resolved stellar populations, which frequently assume a monotonically increasing AMR
A 2-Secure Code with Efficient Tracing Algorithm
A 2-secure code with efficient tracing algorith
The effects of changes in the order of verbal labels and numerical values on children's scores on attitude and rating scales
Research with adults has shown that variations in verbal labels and numerical scale values on rating scales can affect the responses given. However, few studies have been conducted with children. The study aimed to examine potential differences in childrenâs responses to Likert-type rating scales according to their anchor points and scale direction, and to see whether or not such differences were stable over time. 130 British children, aged 9 to 11, completed six sets of Likert-type rating scales, presented in four different ways varying the position of positive labels and numerical values. The results showed, both initially and 8-12 weeks later, that presenting a positive label or a high score on the left of a scale led to significantly higher mean scores than did the other variations. These findings indicate that different arrangements of rating scales can produce different results which has clear implications for the administration of scales with children
The Halo Shape and Evolution of Polar Disc Galaxies
We examine the properties and evolution of a simulated polar disc galaxy.
This galaxy is comprised of two orthogonal discs, one of which contains old
stars (old stellar disc), and the other, containing both younger stars and the
cold gas (polar disc) of the galaxy. By exploring the shape of the inner region
of the dark matter halo, we are able to confirm that the halo shape is a oblate
ellipsoid flattened in the direction of the polar disc. We also note that there
is a twist in the shape profile, where the innermost 3 kpc of the halo flattens
in the direction perpendicular to the old disc, and then aligns with the polar
disc out until the virial radius. This result is then compared to the halo
shape inferred from the circular velocities of the two discs. We also use the
temporal information of the simulation to track the system's evolution, and
identify the processes which give rise to this unusual galaxy type. We confirm
the proposal that the polar disc galaxy is the result of the last major merger,
where the angular moment of the interaction is orthogonal to the angle of the
infalling gas. This merger is followed by the resumption of coherent gas
infall. We emphasise that the disc is rapidly restored after the major merger
and that after this event the galaxy begins to tilt. A significant proportion
of the infalling gas comes from filaments. This infalling gas from the filament
gives the gas its angular momentum, and, in the case of the polar disc galaxy,
the direction of the gas filament does not change before or after the last
major merger.Comment: Accepted for publication in MNRAS; 14 pages; 14 figure
A Large, Uniform Sample of X-ray Emitting AGN from the ROSAT All-Sky and Sloan Digital Sky Surveys: the Data Release 5 Sample
We describe further results of a program aimed to yield ~10^4 fully
characterized optical identifications of ROSAT X-ray sources. Our program
employs X-ray data from the ROSAT All-Sky Survey (RASS), and both optical
imaging and spectroscopic data from the Sloan Digital Sky Survey (SDSS).
RASS/SDSS data from 5740 deg^2 of sky spectroscopically covered in SDSS Data
Release 5 (DR5) provide an expanded catalog of 7000 confirmed quasars and other
AGN that are probable RASS identifications. Again in our expanded catalog, the
identifications as X-ray sources are statistically secure, with only a few
percent of the SDSS AGN likely to be randomly superposed on unrelated RASS
X-ray sources. Most identifications continue to be quasars and Seyfert 1s with
15<m<21 and 0.01<z<4; but the total sample size has grown to include very
substantial numbers of even quite rare AGN, e.g., now including several
hundreds of candidate X-ray emitting BL Lacs and narrow-line Seyfert 1
galaxies. In addition to exploring rare subpopulations, such a large total
sample may be useful when considering correlations between the X-ray and the
optical, and may also serve as a resource list from which to select the "best"
object (e.g., X-ray brightest AGN of a certain subclass, at a preferred
redshift or luminosity) for follow-on X-ray spectral or alternate detailed
studies.Comment: Accepted for publication in AJ; 32 pages, including 11 figures, and 6
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Lonely hearts and angry minds: Online dating rejection increases male (but not female) hostility
The present work explores the hostile tendencies elicited by romantic rejection in the increasingly common context of online dating. To empirically investigate this issue, we created an ad hoc online dating platform in which fictitious online dating partners romantically rejected heterosexual male and female participants. Results revealed that male-but not female-participants who were rejected by desired dating partners displayed increased hostility. This pattern of findings was consistent across different measures, which considered both aggressive tendencies against the rejecting partners and hostile attitudes against the opposite gender. Further, increased feelings of anger explained the relationship between online romantic rejection and increased male hostility. Our work and its findings have both theoretical and methodological implications for the understanding of interpersonal processes in online interactions and the growing body of literature on online dating
Two rapid assays for screening of patulin biodegradation
ArtĂculo sobre distintos ensayos para comprobar la biodegradaciĂłn de la patulinaThe mycotoxin patulin is produced by the blue
mould pathogen Penicillium expansum in rotting apples
during postharvest storage. Patulin is toxic to a wide range
of organisms, including humans, animals, fungi and bacteria.
Wash water from apple packing and processing
houses often harbours patulin and fungal spores, which can
contaminate the environment. Ubiquitous epiphytic yeasts,
such as Rhodosporidium kratochvilovae strain LS11 which
is a biocontrol agent of P. expansum in apples, have the
capacity to resist the toxicity of patulin and to biodegrade
it. Two non-toxic products are formed. One is desoxypatulinic
acid. The aim of the work was to develop rapid,
high-throughput bioassays for monitoring patulin degradation
in multiple samples. Escherichia coli was highly
sensitive to patulin, but insensitive to desoxypatulinic acid.
This was utilized to develop a detection test for patulin,
replacing time-consuming thin layer chromatography or
high-performance liquid chromatography. Two assays for patulin degradation were developed, one in liquid medium
and the other in semi-solid medium. Both assays allow the
contemporary screening of a large number of samples. The
liquid medium assay utilizes 96-well microtiter plates and
was optimized for using a minimum of patulin. The semisolid
medium assay has the added advantage of slowing
down the biodegradation, which allows the study and isolation
of transient degradation products. The two assays are
complementary and have several areas of utilization, from
screening a bank of microorganisms for biodegradation
ability to the study of biodegradation pathways
Parity Violation in Proton-Proton Scattering at 221 MeV
TRIUMF experiment 497 has measured the parity violating longitudinal
analyzing power, A_z, in pp elastic scattering at 221.3 MeV incident proton
energy. This paper includes details of the corrections, some of magnitude
comparable to A_z itself, required to arrive at the final result. The largest
correction was for the effects of first moments of transverse polarization. The
addition of the result, A_z=(0.84 \pm 0.29 (stat.) \pm 0.17 (syst.)) \times
10^{-7}, to the pp parity violation experimental data base greatly improves the
experimental constraints on the weak meson-nucleon coupling constants
h^{pp}_\rho and h^{pp}_\omega, and has implications for the interpretation of
electron parity violation experiments.Comment: 17 pages RevTeX, 14 PostScript figures. Revised version with
additions suggested by Phys. Rev.
Disease self-management needs of adolescents with cancer: perspectives of adolescents with cancer and their parents and healthcare providers
Abstract Purpose The ability for adolescents with cancer (AWC) to engage in disease self-management may result in improved cancer outcomes and quality-of-life ratings for this group. Despite this, a comprehensive self-management program for this group is yet to be developed. To ensure that selfmanagement programming developed for AWC meets the needs of this group, discussion with key stakeholders (i.e., AWC, parents, and healthcare providers) is required. Methods A descriptive qualitative design was used. Adolescents (n029) who varied in age (12 to 18 years) and type of cancer, their parents (n030) and their healthcare providers (n022) were recruited from one large tertiary-care oncology center. Audio-taped semi-structured individual and focusgroup interviews were conducted with participants. Transcribed data were organized into categories that reflected emerging themes. Results Four major themes, which captured the selfmanagement needs of AWC, emerged from the data. These themes were: (1) disease knowledge and cancer care skills, (2) knowledge and skills to support effective transition to adult healthcare, (3) delivery of AWC-accessible healthcare services, and (4) supports for the adolescent with cancer. Conclusions In order to provide comprehensive, relevant, and acceptable self-management programs to AWC, the voices of this population, their parents, and healthcare providers should be considered. Findings from this study will be used to develop and evaluate cancer self-management programming for AWC. Implications for cancer survivors Self-management represents an important avenue for exploration into improving cancer outcomes and quality of life for survivors of cancers during adolescence
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