6,712 research outputs found
High-energy particle transport in 3D hydrodynamic models of colliding-wind binaries
Massive stars in binary systems (as WR140, WR147 or Carinae) have long
been regarded as potential sources of high-energy -rays. The emission
is thought to arise in the region where the stellar winds collide and produce
relativistic particles which subsequently might be able to emit -rays.
Detailed numerical hydrodynamic simulations have already offered insight in the
complex dynamics of the wind collision region (WCR), while independent
analytical studies, albeit with simplified descriptions of the WCR, have shed
light on the spectra of charged particles. In this paper, we describe a
combination of these two approaches. We present a 3D-hydrodynamical model for
colliding stellar winds and compute spectral energy distributions of
relativistic particles for the resulting structure of the WCR. The hydrodynamic
part of our model incorporates the line-driven acceleration of the winds,
gravity, orbital motion and the radiative cooling of the shocked plasma. In our
treatment of charged particles we consider diffusive shock acceleration in the
WCR and the subsequent cooling via inverse Compton losses (including
Klein-Nishina effects), bremsstrahlung, collisions and other energy loss
mechanisms.Comment: 28 pages, 9 figures / accepted for publication in The Astrophysical
Journa
X-ray and gamma-ray orbital variability from the gamma-ray binary HESS J1832-093
Context. Gamma-ray binaries are systems composed of a massive star and a
compact object whose interaction leads to particle acceleration up to
relativistic energies. In the last fifteen years, a few binaries have been
discovered to emit at high energies, but their number is still scarce. The TeV
source HESS J1832-093 has been proposed as a binary candidate, although its
nature is unclear. Neither a GeV counterpart nor a period was found for it.
Aims. The purpose of this work is to search for a gamma-ray source at GeV
energies to understand the origin of the TeV signal. For an unambiguous
identification of its binary nature, finding an orbital modulation is crucial.
Methods. We have analysed data spanning more than 10 years from the Fermi Large
Area Telescope (Fermi-LAT), together with Swift archival observations taken
between 2015 and 2018, using both the X-Ray Telescope (XRT) and UltraViolet and
Optical Telescope (UVOT). We searched for periodicities in both X-ray and
gamma-ray bands using a Lomb-Scargle periodogram. Results. We find a periodic
modulation of \sim 86 days in the X-ray source XMMU J183245-0921539, together
with indications of gamma-ray modulation with a compatible period in 4FGL
J1832.9-0913. Neither an optical nor an UV counterpart is found at the X-ray
source location. The overall spectral energy distribution strongly resembles
the known gamma-ray binary HESS J0632+057. Conclusions. Both the spectrum and
the discovery of an orbital period allow the identification of the TeV source
HESS J1832-093 as a new member of the gamma-ray binary class.Comment: 9 pages, 9 figures. Accepted by A&
A candidate gamma-ray pulsar in the supernova remnant CTA 1
We present a detailed analysis of the high energy gamma-ray source 2EG
J0008+7307. The source has a steady flux and a hard spectrum, softening above 2
GeV. The properties of the gamma-ray source are suggestive of emission from a
young pulsar in the spatially coincident CTA 1 supernova remnant, which has
recently been found to have a non-thermal X-ray plerion. Our 95% uncertainty
contour around the >1 GeV source position includes the point-like X-ray source
at the centre of the plerion. We propose that this object is a young pulsar and
is the most likely counterpart of 2EG J0008+7307.Comment: Accepted for publication in MNRAS. 6 pages including four PS figures.
Uses mn.te
OTV bearing deflection investigation
The primary goal of the Bearing Deflectometer Investigation was to gain experience in the use of fiber optic displacement probe technology for bearing health monitoring in a liquid hydrogen turbo pump. The work specified in this Task Order was conducted in conjunction with Air Force Rocket Propulsion Laboratory Contract F04611-86-C-0010. APD conducted the analysis and design coordination to provide a displacement probe design compatible with the XLR-134 liquid hydrogen turbo pump assembly (TPA). Specifications and requirements of the bearing deflectometer were established working with Mechanical Technology Instruments, Inc. (MTI). The TPA design accommodated positioning of the probe to measure outer race cyclic deflections of the pump inlet bearing. The fiber optic sensor was installed as required in the TPA and sensor output was recorded during the TPA testing. Data review indicated that no bearing deflection signature could be differentiated from the inherent system noise. Alternate sensor installations were not investigated, but might yield different results
Non-adiabatic effects in periodically driven-dissipative open quantum systems
We present a general method to calculate the quasi-stationary state of a
driven-dissipative system coupled to a transmission line (and more generally,
to a reservoir) under periodic modulation of its parameters. Using Floquet's
theorem, we formulate the differential equation for the system's density
operator which has to be solved for a single period of modulation. On this
basis we also provide systematic expansions in both the adiabatic and
high-frequency regime. Applying our method to three different systems -- two-
and three-level models as well as the driven nonlinear cavity -- we propose
periodic modulation protocols of parameters leading to a temporary suppression
of effective dissipation rates, and study the arising non-adiabatic features in
the response of these systems.Comment: 12 pages, 8 figure
Who Should be Interviewed in Surveys of Household Income?
This study tests the null hypothesis that it is sufficient to interview only the household head to obtain accurate information on household income. Results show that using a husband’s estimate of his wife’s income does not produce statistically reliable results for poverty analysis. Estimates of the wife’s income provided by the husband and wife are in agreement in only six percent of households. While limiting interviews to one person has the advantage of reducing the time and expense of household surveys, this appears detrimental in terms of accuracy, and may lead to incorrect conclusions on the determinants of poverty.Africa, gender, household dynamics, household surveys, Malawi, poverty, Agricultural Finance,
The Monoceros very-high-energy gamma-ray source
The H.E.S.S. telescope array has observed the complex Monoceros Loop
SNR/Rosette Nebula region which contains unidentified high energy EGRET sources
and potential very-high-energy (VHE) gamma-ray source. We announce the
discovery of a new point-like VHE gamma-ray sources, HESS J0632+057. It is
located close to the rim of the Monoceros SNR and has no clear counterpart at
other wavelengths. Data from the NANTEN telescope have been used to investigate
hadronic interactions with nearby molecular clouds. We found no evidence for a
clear association. The VHE gamma-ray emission is possibly associated with the
lower energy gamma-ray source 3EG J0634+0521, a weak X-ray source 1RXS
J063258.3+054857 and the Be-star MWC 148.Comment: 4 pages, 4 figures, Contribution to the 30th ICRC, Merida Mexico,
July 200
SHCal13 Southern Hemisphere calibration, 0–50,000 years cal BP
The Southern Hemisphere SHCal04 radiocarbon calibration curve has been updated with the addition of new data sets extending measurements to 2145 cal BP and including the ANSTO Younger Dryas Huon pine data set. Outside the range of measured data, the curve is based upon the Northern Hemisphere data sets as presented in IntCal13, with an interhemispheric offset averaging 43 ± 23 yr modeled by an autoregressive process to represent the short-term correlations in the offset
SHCal04 Southern Hemisphere Calibration, 0–11.0 cal kyr BP
Recent measurements on dendrochronologically-dated wood from the Southern Hemisphere have shown that there are differences between the structural form of the radiocarbon calibration curves from each hemisphere. Thus, it is desirable, when possible, to use calibration data obtained from secure dendrochronologically-dated wood from the corresponding hemisphere. In this paper, we outline the recent work and point the reader to the internationally recommended data set that should be used for future calibration of Southern Hemisphere ¹⁴C dates
The redshift-dependence of gamma-ray absorption in the environments of strong-line AGN
The case of gamma-ray absorption due to photon-photon pair production of jet
photons in the external photon environment like accretion disk and broad-line
region radiation field of gamma-ray loud active galactic nuclei (AGN) that
exhibit strong emission lines is considered. I demonstrate that this ''local
opacity'', if detected, will almost unavoidably be redshift-dependent in the
sub-TeV range. This introduces non-negligible biases, and complicates
approaches for studying the evolution of the extragalactic background light
with contemporary GeV instruments like e.g. the Gamma-ray Large Area Space
Telescope (GLAST), etc., where the gamma-ray horizon is probed by means of
statistical analysis of absorption features (e.g. Fazio-Stecker relation, etc.)
in AGN spectra at various redshifts. It particularly applies to strong-line
quasars where external photon fields are potentially involved in gamma-ray
production.Comment: 19 pages, 5 figures; accepted for publication in Ap
- …