18,810 research outputs found
Motivating Reason to Slow the Factive Turn in Epistemology
In this paper I give a novel argument for the view that epistemic normative reasons (or evidence) need not be facts. I first argue that the nature of normative reasons is uniform, such that our positions about the factivity of reasons should agree across normative realms –– whether epistemic, moral, practical, or otherwise. With that in mind, I proceed in a somewhat indirect way. I argue that if practical motivating reasons are not factive, then practical normative reasons are not factive. If it is possible to act rationally in the light of a falsehood, as I will say, then some good reasons must be falsehoods. The implication of this argument is perhaps surprising: for one to firmly establish the view that epistemic normative reasons are factive, one must discredit the view that practical motivating reasons are not factive
Origin of asymmetries in X-ray emission lines from the blast wave of the 2014 outburst of nova V745 Sco
The symbiotic nova V745 Sco was observed in outburst on 2014 February 6. Its
observations by the Chandra X-ray Observatory at days 16 and 17 have revealed a
spectrum characterized by asymmetric and blue-shifted emission lines. Here we
investigate the origin of these asymmetries through three-dimensional
hydrodynamic simulations describing the outburst during the first 20 days of
evolution. The model takes into account thermal conduction and radiative
cooling and assumes a blast wave propagates through an equatorial density
enhancement. From the simulations, we synthesize the X-ray emission and derive
the spectra as they would be observed with Chandra. We find that both the blast
wave and the ejecta distribution are efficiently collimated in polar directions
due to the presence of the equatorial density enhancement. The majority of the
X-ray emission originates from the interaction of the blast with the equatorial
density enhancement and is concentrated on the equatorial plane as a ring-like
structure. Our "best-fit" model requires a mass of ejecta in the outburst
and an explosion energy erg and reproduces the distribution of emission
measure vs temperature and the evolution of shock velocity and temperature
inferred from the observations. The model predicts asymmetric and blue-shifted
line profiles similar to those observed and explains their origin as due to
substantial X-ray absorption of red-shifted emission by ejecta material. The
comparison of predicted and observed Ne and O spectral line ratios reveals no
signs of strong Ne enhancement and suggests the progenitor is a CO white dwarf.Comment: 16 pages, 17 Figures; accepted for publication on MNRA
Electrodynamic effects of Jupiter's satellite Io
Electrodynamic effects of Jupiters satellite I
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