4,171 research outputs found
Sensation Seeking and Perceived Need for Structure Moderate Soldiers’ Well-Being Before and After Operational Deployment
This study examined associations between sensation seeking and perceived need for structure, and changes in reported well-being among deployed soldiers. Participants (n = 167) were assessed before and after a six-month deployment to south Afghanistan. Results indicated that although well-being declined in the soldier sample as a whole following deployment, the degree of decrease was significantly different among soldiers with different personality profiles. Differences were moderated by soldiers’ level of sensation seeking and perceived need for structure. Results are discussed in terms of a person-environment fit theory in the context of preparation and rehabilitation of deployed military personnel
Non-LTE models for the gaseous metal component of circumstellar discs around white dwarfs
Gaseous metal discs around single white dwarfs have been discovered recently.
They are thought to develop from disrupted planetary bodies. Spectroscopic
analyses will allow us to study the composition of extrasolar planetary
material. We investigate in detail the first object for which a gas disc was
discovered (SDSS J122859.93+104032.9). Therefor we perform non-LTE modelling of
viscous gas discs by computing the detailed vertical structure and line
spectra. The models are composed of carbon, oxygen, magnesium, silicon,
calcium, and hydrogen with chemical abundances typical for Solar System
asteroids. Line asymmetries are modelled by assuming spiral-arm and eccentric
disc structures as suggested by hydrodynamical simulations. The observed
infrared Ca II emission triplet can be modelled with a hydrogen-deficient metal
gas disc located inside of the tidal disruption radius, with an effective
temperature of about 6000 K and a surface mass density of 0.3 g/cm^2. The inner
radius is well constrained at about 0.64 Solar radii. The line profile
asymmetry can be reproduced by either a spiral-arm structure or an eccentric
disc, the latter being favoured by its time variability behaviour. Such
structures, reaching from 0.64 to 1.5 Solar radii, contain a mass of about 3 to
6*10^21 g, the latter equivalent to the mass of a 135-km diameter Solar System
asteroid.Comment: 7 pages, 10 figures, accepted for publication in A&
Batalin-Vilkovisky Integrals in Finite Dimensions
The Batalin-Vilkovisky method (BV) is the most powerful method to analyze
functional integrals with (infinite-dimensional) gauge symmetries presently
known. It has been invented to fix gauges associated with symmetries that do
not close off-shell. Homological Perturbation Theory is introduced and used to
develop the integration theory behind BV and to describe the BV quantization of
a Lagrangian system with symmetries. Localization (illustrated in terms of
Duistermaat-Heckman localization) as well as anomalous symmetries are discussed
in the framework of BV.Comment: 35 page
The Discovery of a Debris Disk Around the DAV White Dwarf PG 1541+651
To search for circumstellar disks around evolved stars, we targeted roughly
100 DA white dwarfs from the Palomar Green survey with the Peters Automated
Infrared Imaging Telescope (PAIRITEL). Here we report the discovery of a debris
disk around one of these targets, the pulsating white dwarf PG 1541+651 (KX
Draconis, hereafter PG1541). We detect a significant flux excess around PG1541
in the K-band. Follow-up near-infrared spectroscopic observations obtained at
the NASA Infrared Telescope Facility (IRTF) and photometric observations with
the warm Spitzer Space Telescope confirm the presence of a warm debris disk
within 0.13-0.36 Rsun (11-32x the stellar radius) at an inclination angle of
60deg. At Teff = 11880 K, PG1541 is almost a twin of the DAV white dwarf
G29-38, which also hosts a debris disk. All previously known dusty white dwarfs
are of the DAZ/DBZ spectral type due to accretion of metals from the disk.
High-resolution optical spectroscopy is needed to search for metal absorption
lines in PG1541 and to constrain the accretion rate from the disk. PG1541 is
only 55 pc away from the Sun and the discovery of its disk in our survey
demonstrates that our knowledge of the nearby dusty white dwarf population is
far from complete.Comment: MNRAS Letters, in pres
The chemical composition of nearby young associations: s-process element abundances in AB Doradus, Carina-Near, and Ursa Major
Recently, several studies have shown that young, open clusters are
characterised by a considerable over-abundance in their barium content. In
particular, D'Orazi et al. (2009) reported that in some younger clusters
[Ba/Fe] can reach values as high as ~0.6 dex. The work also identified the
presence of an anti-correlation between [Ba/Fe] and cluster age. For clusters
in the age range ~4.5 Gyr-500 Myr, this is best explained by assuming a higher
contribution from low-mass asymptotic giant branch stars to the Galactic
chemical enrichment. The purpose of this work is to investigate the ubiquity of
the barium over-abundance in young stellar clusters. We analysed
high-resolution spectroscopic data, focusing on the s-process elemental
abundance for three nearby young associations, i.e. AB Doradus, Carina-Near,
and Ursa Major. The clusters have been chosen such that their age spread would
complement the D'Orazi et al. (2009) study. We find that while the s-process
elements Y, Zr, La, and Ce exhibit solar ratios in all three associations, Ba
is over-abundant by ~0.2 dex. Current theoretical models can not reproduce this
abundance pattern, thus we investigate whether this unusually large Ba content
might be related to chromospheric effects. Although no correlation between
[Ba/Fe] and several activity indicators seems to be present, we conclude that
different effects could be at work which may (directly or indirectly) be
related to the presence of hot stellar chromospheres.Comment: Accepted for publication in MNRA
HST and Spitzer Observations of the HD 207129 Debris Ring
A debris ring around the star HD 207129 (G0V; d = 16.0 pc) has been imaged in
scattered visible light with the ACS coronagraph on the Hubble Space Telescope
and in thermal emission using MIPS on the Spitzer Space Telescope at 70 microns
(resolved) and 160 microns (unresolved). Spitzer IRS (7-35 microns) and MIPS
(55-90 microns) spectrographs measured disk emission at >28 microns. In the HST
image the disk appears as a ~30 AU wide ring with a mean radius of ~163 AU and
is inclined by 60 degrees from pole-on. At 70 microns it appears partially
resolved and is elongated in the same direction and with nearly the same size
as seen with HST in scattered light. At 0.6 microns the ring shows no
significant brightness asymmetry, implying little or no forward scattering by
its constituent dust. With a mean surface brightness of V=23.7 mag per square
arcsec, it is the faintest disk imaged to date in scattered light.Comment: 28 pages, 8 figure
A Dusty M5 Binary in the beta Pictoris Moving Group
We report the identification of a new wide separation binary (LDS 5606) in
the ~20 Myr-old beta Pic moving group. This M5+M5 pair has a projected
separation of 26'', or ~1700 AU at a distance of 65 pc. Both stars host warm
circumstellar disks and many strong hydrogen and helium emission lines.
Spectroscopic observations reveal signatures of youth for both stars and
on-going mass accretion in the primary. The properties of LDS 5606 make it an
older analog to the ~8 Myr TWA 30 system, which is also composed of a pair of
widely separated mid-M dwarfs, each hosting their own warm circumstellar disks.
LDS 5606 joins a rather exclusive club of only 3 other known stellar systems
where both members of a binary, far from any molecular cloud, are orbited by
detected circumstellar disks.Comment: 8 pages, 6 figures; Accepted for publication in A&
Herbal Product Use Among Anticoagulation Patients
Warfarin interacts with many conventional drug products and herbal products,1-3 Given the incompleteness of information on drug-herbal product interactions and the potential for health care practitioners to be unaware of their patients\u27 utilization of herbal products, we surveyed the use of such products among patients receiving warfarin through an anticoagulation clinic. Patients at the University of Maryland Medical System Anticoagulation Clinic were asked to complete an anonymous written questionnaire during their regularly scheduled appointments over one month
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