7,180 research outputs found
XMM-Newton observations of SDSS J143030.22001115.1: an unusually flat spectrum AGN
We present XMM observations of the AGN SDSS 1430-0011. The low S/N spectrum
of this source obtained in a snap shot Chandra observation showed an unusually
flat continuum. With the follow up XMM observations we find that the source
spectrum is complex; it either has an ionized absorber or a partially covering
absorber. The underlying power-law is in the normal range observed for AGNs.
The low luminosity of the source during Chandra observations can be understood
in terms of variations in the absorber properties. The X-ray and optical
properties of this source are such that it cannot be securely classified as
either a narrow line Seyfert 1 or a broad line Seyfert 1 galaxy.Comment: Submitted to A
Radioactive Iron Rain: Transporting Fe in Supernova Dust to the Ocean Floor
Several searches have found evidence of Fe deposition, presumably from
a near-Earth supernova (SN), with concentrations that vary in different
locations on Earth. This paper examines various influences on the path of
interstellar dust carrying Fe from a SN through the heliosphere, with
the aim of estimating the final global distribution on the ocean floor. We
study the influences of magnetic fields, angle of arrival, wind and ocean
cycling of SN material on the concentrations at different locations. We find
that the passage of SN material through the mesosphere/lower thermosphere (MLT)
is the greatest influence on the final global distribution, with ocean cycling
causing lesser alteration as the SN material sinks to the ocean floor. SN
distance estimates in previous works that assumed a uniform distribution are a
good approximation. Including the effects on surface distributions, we estimate
a distance of pc for a SN progenitor. This
is consistent with a SN occurring within the Tuc-Hor stellar group 2.8
Myr ago with SN material arriving on Earth 2.2 Myr ago. We note that the
SN dust retains directional information to within through its
arrival in the inner Solar System, so that SN debris deposition on inert bodies
such as the Moon will be anisotropic, and thus could in principle be used to
infer directional information. In particular, we predict that existing lunar
samples should show measurable Fe differences.Comment: 18 pages, 8 figures. Comments welcom
Astrophysical Shrapnel: Discriminating Among Near-Earth Stellar Explosion Sources of Live Radioactive Isotopes
We consider the production and deposition on Earth of isotopes with
half-lives in the range 10 to 10 years that might provide
signatures of nearby stellar explosions, extending previous analyses of
Core-Collapse Supernovae (CCSNe) to include Electron-Capture Supernovae
(ECSNe), Super-Asymptotic Giant Branch (SAGBs) stars, Thermonuclear/Type Ia
Supernovae (TNSNe), and Kilonovae/Neutron Star Mergers (KNe). We revisit
previous estimates of the Fe and Al signatures, and extend these
estimates to include Pu and Mn. We discuss interpretations of
the Fe signals in terrestrial and lunar reservoirs in terms of a nearby
stellar ejection ~2.2 Myr ago, showing that (i) the Fe yield rules out
the TNSN and KN interpretations, (ii) the Fe signals highly constrain a
SAGB interpretation but do not completely them rule out, (iii) are consistent
with a CCSN origin, and (iv) are highly compatible with an ECSN interpretation.
Future measurements could resolve the radioisotope deposition over time, and we
use the Sedov blast wave solution to illustrate possible time-resolved
profiles. Measuring such profiles would independently probe the blast
properties including distance, and would provide additional constraints the
nature of the explosion.Comment: 38 pages, 6 figures. Comments welcom
Bell's Theorem from Moore's Theorem
It is shown that the restrictions of what can be inferred from
classically-recorded observational outcomes that are imposed by the no-cloning
theorem, the Kochen-Specker theorem and Bell's theorem also follow from
restrictions on inferences from observations formulated within classical
automata theory. Similarities between the assumptions underlying classical
automata theory and those underlying universally-unitary quantum theory are
discussed.Comment: 12 pages; to appear in Int. J. General System
Comparison of measured and calculated temperatures for a Mach 8 hypersonic wing test structure
Structural temperatures were measured on a hypersonic wing test structure during a heating test that simulated a Mach 8 thermal environment. Measured data are compared to design calculations and temperature predictions obtained from a finite-difference thermal analysis
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