9,874 research outputs found
The casting and powder-metallurgy forming of precipitation-hardenable stainless steels
Casting and powder metallurgy techniques for shaping precipitation hardened stainless steel
Dissecting the Power Sources of Low-Luminosity Emission-Line Galaxy Nuclei via Comparison of HST-STIS and Ground-Based Spectra
Using a sample of ~100 nearby line-emitting galaxy nuclei, we have built the
currently definitive atlas of spectroscopic measurements of H_alpha and
neighboring emission lines at subarcsecond scales. We employ these data in a
quantitative comparison of the nebular emission in Hubble Space Telescope (HST)
and ground-based apertures, which offer an order-of-magnitude difference in
contrast, and provide new statistical constraints on the degree to which
Transition Objects and low-ionization nuclear emission-line regions (LINERs)
are powered by an accreting black hole at <10 pc. We show that while the
small-aperture observations clearly resolve the nebular emission, the aperture
dependence in the line ratios is generally weak, and this can be explained by
gradients in the density of the line-emitting gas: the higher densities in the
more nuclear regions potentially flatten the excitation gradients, suppressing
the forbidden emission. The Transition Objects show a threefold increase in the
incidence of broad H_alpha emission in the high-resolution data, as well as the
strongest density gradients, supporting the composite model for these systems
as accreting sources surrounded by star-forming activity. The narrow-line
LINERs appear to be the weaker counterparts of the Type 1 LINERs, where the low
accretion rates cause the disappearance of the broad-line component. The
enhanced sensitivity of the HST observations reveals a 30% increase in the
incidence of accretion-powered systems at z~0. A comparison of the strength of
the broad-line emission detected at different epochs implies potential
broad-line variability on a decade-long timescale, with at least a factor of
three in amplitude.Comment: 27 pages, 13 figures, 4 tables, accepted for publication in Ap
Addendum to `Fake Projective Planes'
The addendum updates the results presented in the paper `Fake Projective
Plane, Invent Math 168, 321-370 (2007)' and makes some additions and
corrections. The fake projective planes are classified into twenty six classes.
Together with a recent work of Donald Cartwright and Tim Steger, there is now a
complete list of fake projective planes. There are precisely one hundred fake
projective planes as complex surfaces classified up to biholomorphism.Comment: A more refined classification is given in the new versio
Measurement of gamma p --> K+ Lambda and gamma p --> K+ Sigma0 at photon energies up to 2.6 GeV
The reactions gamma p --> K+ Lambda and gamma p --> K+ Sigma0 were measured
in the energy range from threshold up to a photon energy of 2.6 GeV. The data
were taken with the SAPHIR detector at the electron stretcher facility, ELSA.
Results on cross sections and hyperon polarizations are presented as a function
of kaon production angle and photon energy. The total cross section for Lambda
production rises steeply with energy close to threshold, whereas the Sigma0
cross section rises slowly to a maximum at about E_gamma = 1.45 GeV. Cross
sections together with their angular decompositions into Legendre polynomials
suggest contributions from resonance production for both reactions. In general,
the induced polarization of Lambda has negative values in the kaon forward
direction and positive values in the backward direction. The magnitude varies
with energy. The polarization of Sigma0 follows a similar angular and energy
dependence as that of Lambda, but with opposite sign.Comment: 21 pages, 25 figures, submitted to Eur. Phys. J.
Polarized Broad-Line Emission from Low-Luminosity Active Galactic Nuclei
In order to determine whether unified models of active galactic nuclei apply
to low-luminosity objects, we have undertaken a spectropolarimetric survey of
of LINERs and Seyfert nuclei at the Keck Observatory. The 14 objects observed
have a median H-alpha luminosity of 8x10^{39} erg/s, well below the typical
value of ~10^{41} erg/s for Markarian Seyfert nuclei. Polarized broad H-alpha
emission is detected in three LINERs: NGC 315, NGC 1052, and NGC 4261. Each of
these is an elliptical galaxy with a double-sided radio jet, and the
emission-line polarization in each case is oriented roughly perpendicular to
the jet axis, as expected for the obscuring torus model. NGC 4261 and NGC 315
are known to contain dusty circumnuclear disks, which may be the outer
extensions of the obscuring tori. The detection of polarized broad-line
emission suggests that these objects are nearby, low-luminosity analogs of
obscured quasars residing in narrow-line radio galaxies. The nuclear continuum
of the low-luminosity Seyfert 1 galaxy NGC 4395 is polarized at p = 0.67%,
possibly the result of an electron scattering region near the nucleus.
Continuum polarization is detected in other objects, with a median level of p =
0.36% over 5100-6100 A, but in most cases this is likely to be the result of
transmission through foreground dust. The lack of significant broad-line
polarization in most type 1 LINERs is consistent with the hypothesis that we
view the broad-line regions of these objects directly, rather than in scattered
light.Comment: 28 pages, including 3 tables and 16 figures. Uses the emulateapj
latex style file. Accepted for publication in The Astrophysical Journa
The making of nickel and nickel-alloy shapes by casting, powder metallurgy, electroforming, chemical vapor deposition, and metal spraying
Casting, powder metallurgy, electroforming, metal spraying, and chemical vapor deposition techniques for producing nickel and nickel-alloy shape
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