175 research outputs found
Development of procedures for calculating stiffness and damping of elastomers in engineering applications. Part 5: Elastomer performance limits and the design and test of an elastomer damper
Tests were performed on elastomer specimens of the material polybutadiene to determine the performance limitations imposed by strain, temperature, and frequency. Three specimens were tested: a shear specimen, a compression specimen, and a second compression specimen in which thermocouples were embedded in the elastomer buttons. Stiffness and damping were determined from all tests, and internal temperatures were recorded for the instrumented compression specimen. Measured results are presented together with comparisons between predictions of a thermo-viscoelastic analysis and the measured results. Dampers of polybutadiene and Viton were designed, built, and tested. Vibration measurements were made and sensitivity of vibration to change in unbalance was also determined. Values for log decrement were extracted from the synchronous response curves. Comparisons were made between measured sensitivity to unbalance and log decrement and predicted values for these quantities
Resolving Star Formation on Sub-Kiloparsec Scales in the High-Redshift Galaxy SDP.11 Using Gravitational Lensing
We investigate the properties of the interstellar medium, star formation, and
the current-day stellar population in the strongly-lensed star-forming galaxy
H-ATLAS J091043.1-000321 (SDP.11), at z = 1.7830, using new Herschel and ALMA
observations of far-infrared fine-structure lines of carbon, oxygen and
nitrogen. We report detections of the [O III] 52 um, [N III] 57 um, and [O I]
63 um lines from Herschel/PACS, and present high-resolution imaging of the [C
II] 158 um line, and underlying continuum, using ALMA. We resolve the [C II]
line emission into two spatially-offset Einstein rings, tracing the red- and
blue-velocity components of the line, in the ALMA/Band-9 observations at 0.2"
resolution. The values seen in the [C II]/FIR ratio map, as low as ~ 0.02% at
the peak of the dust continuum, are similar to those of local ULIRGs,
suggesting an intense starburst in this source. This is consistent with the
high intrinsic FIR luminosity (~ 3 x 10^12 Lo), ~ 16 Myr gas depletion
timescale, and < 8 Myr timescale since the last starburst episode, estimated
from the hardness of the UV radiation field. By applying gravitational lensing
models to the visibilities in the uv-plane, we find that the lensing
magnification factor varies by a factor of two across SDP.11, affecting the
observed line profiles. After correcting for the effects of differential
lensing, a symmetric line profile is recovered, suggesting that the starburst
present here may not be the result of a major merger, as is the case for local
ULIRGs, but instead could be powered by star-formation activity spread across a
3-5 kpc rotating disk.Comment: 17 pages, 8 figures, 3 tables, accepted for publication in the
Astrophysical Journa
Optical integral field spectroscopy of intermediate redshift infrared bright galaxies
The extreme infrared (IR) luminosity of local luminous and ultra-luminous IR
galaxies (U/LIRGs; 11 12,
respectively) is mainly powered by star-formation processes triggered by
mergers or interactions. While U/LIRGs are rare locally, at z > 1, they become
more common, they dominate the star-formation rate (SFR) density, and a
fraction of them are found to be normal disk galaxies. Therefore, there must be
an evolution of the mechanism triggering these intense starbursts with
redshift. To investigate this evolution, we present new optical SWIFT integral
field spectroscopic H{\alpha}+[NII] observations of a sample of 9
intermediate-z (0.2 < z < 0.4) U/LIRG systems selected from Herschel 250{\mu}m
observations. The main results are the following: (a) the ratios between the
velocity dispersion and the rotation curve amplitude indicate that 10-25% (1-2
out of 8) might be compatible with being isolated disks while the remaining
objects are interacting/merging systems; (b) the ratio between un-obscured and
obscured SFR traced by H{\alpha} and LIR, respectively, is similar in both
local and these intermediate-z U/LIRGs; and (c) the ratio between 250{\mu}m and
the total IR luminosities of these intermediate-z U/LIRGs is higher than that
of local U/LIRGs with the same LIR . This indicates a reduced dust temperature
in these intermediate-z U/LIRGs. This, together with their already measured
enhanced molecular gas content, suggests that the interstellar medium
conditions are different in our sample of intermediate-z galaxies when compared
to local U/LIRGs.Comment: Accepted for publication in MNRA
Intense Star-formation and Feedback at High Redshift: Spatially-resolved Properties of the z=2.6 Submillimeter Galaxy SMMJ14011+0252
We present a detailed analysis of the spatially-resolved properties of the
lensed submillimeter galaxy SMMJ14011+0252 at z=2.56, combining deep
near-infrared integral-field data obtained with SPIFFI on the VLT with other
multi-wavelength data sets. The broad characteristics of SMMJ14011+0252 are in
agreement with what is expected for the early evolution of local massive
spheroidal galaxies. From continuum and line flux, velocity, and dispersion
maps, we measure the kinematics, star-formation rates, gas densities, and
extinction for individual subcomponents. The star formation intensity is
similar to low-redshift ``maximal starbursts'', while the line fluxes and the
dynamics of the emission line gas provide direct evidence for a
starburst-driven wind with physical properties very similar to local
superwinds. We also find circumstantial evidence for "self-regulated" star
formation within J1. The relative velocity of the bluer companion J2 yields a
dynamical mass estimate for J1 within about 20 kpc, M_dyn \sim 1\times 10^{11}
M_sun. The relative metallicity of J2 is 0.4 dex lower than in J1n/s,
suggesting different star formation histories. SED fitting of the continuum
peak J1c confirms and substantiates previous suggestions that this component is
a z=0.25 interloper. When removing J1c, the stellar continuum and H-alpha line
emission appear well aligned spatially in two individual components J1n and
J1s, and coincide with two kinematically distinct regions in the velocity map,
which might well indicate a merging system. This highlights the close
similarity between SMGs and ULIRGs, which are often merger-driven maximal
starbursts, and suggests that the intrinsic mechanisms of star-formation and
related feedback are similar to low-redshift strongly star-forming systems.Comment: Some of the figures changed from b/w to colo
Gas Dynamics in the Luminous Merger NGC 6240
We report 0.5"x0.9" resolution, interferometric observations of the 1.3 mm CO
J=2-1 line in the infrared luminous galactic merger NGC 6240. About half of the
CO flux is concentrated in a rotating but highly turbulent, thick disk
structure centered between the two radio and near-infrared nuclei. A number of
gas features connect this ~500 pc diameter central disk to larger scales.
Throughout this region the molecular gas has local velocity widths which exceed
300 km/s FWHM and even reach FWZP line widths of 1000 km/s in a number of
directions. The mass of the central gas concentration constitutes a significant
fraction of the dynamical mass, M_gas(R<470 pc) ~ 2-4x10^9 M_o ~ 0.3-0.7 M_dyn.
We conclude that NGC 6240 is in an earlier merging stage than the prototypical
ultraluminous galaxy, Arp 220. The interstellar gas in NGC 6240 is in the
process of settling between the two progenitor stellar nuclei, is dissipating
rapidly and will likely form a central thin disk. In the next merger stage, NGC
6240 may well experience a major starburst like that observed in Arp 220.Comment: To be published in Ap.J.; 7 figure
Stellar Dynamics and the implications on the merger evolution in NGC6240
We report near-infrared integral field spectroscopy of the luminous merging
galaxy NGC 6240. Stellar velocities show that the two K-band peaks separated by
1.6arcsec are the central parts of inclined, rotating disk galaxies with equal
mass bulges. The dynamical masses of the nuclei are much larger than the
stellar mass derived from the K-band light, implying that the progenitor
galaxies were galaxies with massive bulges. The K-band light is dominated by
red supergiants formed in the two nuclei in starbursts, triggered ~2x10^7 years
ago, possibly by the most recent perigalactic approach. Strong feedback effects
of a superwind and supernovae are responsible for a short duration burst
(~5x10^6 years) which is already decaying. The two galaxies form a
prograde-retrograde rotating system and from the stellar velocity field it
seems that one of the two interacting galaxies is subject to a prograde
encounter. Between the stellar nuclei is a prominent peak of molecular gas
(H_2, CO). The stellar velocity dispersion peaks there indicating that the gas
has formed a local, self-gravitating concentration decoupled from the stellar
gravitational potential. NGC 6240 has previously been reported to fit the
paradigm of an elliptical galaxy formed through the merger of two galaxies.
This was based on the near-infrared light distribution which follows a
r^1/4-law. Our data cast strong doubt on this conclusion: the system is by far
not relaxed, rotation plays an important role, as does self-gravitating gas,
and the near-infrared light is dominated by young stars.Comment: 34 pages, 11 figures, using AASTEX 5.0rc3.1, paper submitted to the
Astrophysical Journal, revised versio
¿Qué leían los cruzados argentinos? : Las lecturas del nacionalismo católico a través de 'Cabildo' (1973-1976)
En el siguiente artículo se aborda la revista nacionalista católica Cabildo desde una perspectiva sensible a la historia intelectual. El objetivo es ampliar y completar, a partir de las lecturas promocionadas en las publicidades y de los libros reseñados, el universo de representaciones políticas y religiosas. Luego de presentar la revista, largamente estudiada por la historiografía, se analizan las publicidades identificando redes intelectuales locales, pero también transnacionales. En forma posterior se examinan tres reseñas dedicadas a la lectura de la historia, la ciencia ficción y la guerra contrarrevolucionaria. Se concluye que el nacionalismo católico, lejos de impugnar la modernidad en un nivel ontológico, trazó un diálogo práctico bajo la condición de corregir sus peligrosas derivas.En el següent article s'aborda la revista nacionalista catòlica Cabildo des d'una perspectiva sensible a la història intel·lectual. L'objectiu és ampliar i completar, a partir de les lectures promocionades en les publicitats i dels llibres ressenyats, l'univers de representacions polítiques i religioses. Després de presentar la revista, llargament estudiada per la historiografia, s'analitzen les publicitats tot identificant xarxes intel·lectuals locals, però també transnacionals. Més endavant s'examinen tres ressenyes dedicades a la lectura de la història, la ciència-ficció i la guerra contrarevolucionària. Es conclou que el nacionalisme catòlic, lluny d'impugnar la modernitat en un nivell ontològic, va traçar un diàleg pràctic sota la condició de corregir les seves perilloses derives.The following paper focuses on the Catholic nationalist magazine Cabildo from an Intellectual History standpoint. The aim is to expand and complete, from the reading matter promoted in its advertisements and the books reviewed, the universe of its political and religious representations. After a brief introduction to the magazine, long studied in the literature, the advertisements are analyzed and transnational as well as local intellectual networks are identified. Later, three book reviews, focusing on the interpretation of Argentine history, science fiction, and the counterrevolutionary war, are examined. It is concluded that, far from challenging modernity on an ontological level, Cabildo entered into a practical dialogue with it without accepting its dangerous deviations
Ultr-Luminous Infrared Galaxies: QSOs in Formation?
We present new near-infrared Keck and VLT spectroscopic data on the stellar
dynamics in late stage, ultra-luminous infrared galaxy (ULIRG) mergers . We now
have information on the structural and kinematic properties of 18 ULIRGs, 8 of
which contain QSO-like active galactic nuclei. The host properties (velocity
dispersion, effective radius, effective surface brightness, M_K) of
AGN-dominated and star formation dominated ULIRGs are similar. ULIRGs fall
remarkably close to the fundamental plane of early type galaxies. They populate
a wide range of the plane, are on average similar to L*-rotating ellipticals,
but are well offset from giant ellipticals and optically/UV bright, low-z
QSOs/radio galaxies. ULIRGs and local QSOs/radio galaxies are very similar in
their distributions of bolometric and extinction corrected near-IR
luminosities, but ULIRGs have smaller effective radii and velocity dispersions
than the local QSO/radio galaxy population. Hence, their host masses and
inferred black hole masses are correspondingly smaller. The latter are more
akin to those of local Seyfert galaxies. ULIRGs thus resemble local QSOs in
their near-IR and bolometric luminosities because they are (much more)
efficiently forming stars and/or feeding their black holes, and not because
they have QSO-like, very massive black holes. We conclude that ULIRGs as a
class cannot evolve into optically bright QSOs. They will more likely become
quiescent, moderate mass field ellipticals or, when active, might resemble the
X-ray bright, early type galaxies that have recently been found by the Chandra
Observatory.Comment: accepted to be published in ApJ, 7 figure
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