9,628 research outputs found
Black hole hunting in the Andromeda Galaxy
We present a new technique for identifying stellar mass black holes in low
mass X-ray binaries (LMXBs), and apply it to XMM-Newton observations of M31. We
examine X-ray time series variability seeking power density spectra (PDS)
typical of LMXBs accreting at a low accretion rate (which we refer to as Type A
PDS); these are very similar for black hole and neutron star LMXBs. Galactic
neutron star LMXBs exhibit Type A PDS at low luminosities (~10^36--10^37 erg/s)
while black hole LMXBs can exhibit them at luminosities >10^38 erg/s. We
propose that Type A PDS are confined to luminosities below a critical fraction
of the Eddington limit, that is constant for all LMXBs; we have examined
asample of black hole and neutron star LMXBs and find they are all consistent
with = 0.10+/-0.04 in the 0.3--10 keV band. We present luminosity and PDS
data from 167 observations of X-ray binaries in M31 that provide strong support
for our hypothesis. Since the theoretical maximum mass for a neutron star is
\~3.1 M_Sun, we therefore assert that any LMXB that exhibits a Type A PDS at a
0.3--10 keV luminosity greater than 4 x 10^37 erg/s is likely to contain a
black hole primary. We have found eleven new black hole candidates in M31 using
this method. We focus on XMM-Newton observations of RX J0042.4+4112, an X-ray
source in M31 and find the mass of the primary to be 7+/-2 M_Sun, if our
assumptions are correct. Furthermore, RX J0042.4+4112 is consistently bright in
\~40 observations made over 23 years, and is likely to be a persistently bright
LMXB; by contrast all known Galactic black hole LMXBs are transient. Hence our
method may be used to find black holes in known, persistently bright Galactic
LMXBs and also in LMXBs in other galaxies.Comment: 6 Pages, 6 figures. To appear in the conference proceedings of
"Interacting Binaries: Accretion, Evolution and Outcomes" (Cefalu, July 4-10
2004
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EU Employment Law and the European Social Model: The Past, the Present and the Future
If the critics are right, the European Union’s (EU’s) social model is dead and that is the end of it. Those on the right may well be dancing on its grave; those more sympathetic might mourn its passing. My view is more sanguine. I shall argue that the European social model is certainly facing unprecedented challenges. However, I will suggest that these challenges, caused in part by the EU’s response to the crisis but more generally resulting from a growing hostility towards the European Union project as a whole, are not terminal and that there is—and should be—a continued role for the European social model. The article therefore considers what is meant by the European social model (ESM) and why the ESM is important. It then examines why the ESM, and its employment dimension in particular, is facing such difficulties before recognizing that, in fact, the EU’s history demonstrates that the ESM has, in fact, a long-standing ability to regenerate and resurrect itself in different guises. Given this regenerative capacity, the article will conclude by considering the form EU social policy might take going forward.This is the author accepted manuscript. The final version is available from Oxford University Press via http://dx.doi.org/10.1093/clp/cuu01
Evolution of correlation strength in KxFe(2-y)Se2 superconductor doped with S
We report the evolution of thermal transport properties of iron-based
superconductor KFeSe with sulfur substitution at Se sites.
Sulfur doping suppresses the superconducting as well as the Seebeck
coefficient. The Seebeck coefficient of all crystals in the low temperature
range can be described very well by diffusive thermoelectric response model.
The zero-temperature extrapolated value of Seebeck coefficient divided by
temperature gradually decreases from to a very small
value 0.03 V/K where is completely suppressed. The normal
state electron Sommerfeld term () of specific heat also decreases
with the increase of sulfur content. The dcrease of and
reflects a suppression of the density of states at the Fermi energy, or a
change in the Fermi surface that would induce the suppression of correlation
strength.Comment: 5 Pages, 4 figures, 1 Table; submitted to Physical Review
Systems, interactions and macrotheory
A significant proportion of early HCI research was guided by one very clear vision: that the existing theory base in psychology and cognitive science could be developed to yield engineering tools for use in the interdisciplinary context of HCI design. While interface technologies and heuristic methods for behavioral evaluation have rapidly advanced in both capability and breadth of application, progress toward deeper theory has been modest, and some now believe it to be unnecessary. A case is presented for developing new forms of theory, based around generic “systems of interactors.” An overlapping, layered structure of macro- and microtheories could then serve an explanatory role, and could also bind together contributions from the different disciplines. Novel routes to formalizing and applying such theories provide a host of interesting and tractable problems for future basic research in HCI
Thermoelectric studies of KxFe2-ySe2: weakly correlated superconductor
We report thermal transport measurement of KxFe2-ySe2 superconducting single
crystal. Significant peak anomaly in thermal conductivity is observed at nearly
TC/2 indicating a large phonon mean-free-path in the superconducting state. The
zero-temperature extrapolated thermoelectric power is smaller than the value in
typical strongly correlated superconductors, implying large normalized Fermi
temperature. In contrast to other iron superconductors, thermoelectric power in
our sample does not exhibit significant anomalies. These findings indicate that
KxFe2-ySe2 is a weakly or intermediately correlated superconductor without
significant Fermi surface nesting.Comment: Revised version, 5 pages, 5 figures, Will appear in Physical Review
Cumulative luminosity functions of the X-ray point source population in M31
We present preliminary results from a detailed analysis of the X-ray point
sources in the XMM-Newton survey of M31. These sources are expected to be
mostly X-ray binaries. We have so far studied 225 of the 535 sources found by
automated source detection. Only sources which were present in all three EPIC
images were considered. X-ray binaries are identified by their energy spectrum
and power density spectrum. Unlike in other surveys we have obtained source
luminosities from freely fit emission models. We present uncorrected luminosity
functions of the sources analysed so far.Comment: 2 pages, 1 figure. To appear in proceedings of IAUS23
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