26,669 research outputs found
The Musca cloud: A 6 pc-long velocity-coherent, sonic filament
Filaments play a central role in the molecular clouds' evolution, but their
internal dynamical properties remain poorly characterized. To further explore
the physical state of these structures, we have investigated the kinematic
properties of the Musca cloud. We have sampled the main axis of this
filamentary cloud in CO and CO (2--1) lines using APEX
observations. The different line profiles in Musca shows that this cloud
presents a continuous and quiescent velocity field along its 6.5 pc of
length. With an internal gas kinematics dominated by thermal motions (i.e.,
) and large-scale velocity gradients, these results
reveal Musca as the longest velocity-coherent, sonic-like object identified so
far in the ISM. The transonic properties of Musca present a clear departure
from the predicted supersonic velocity dispersions expected in the Larson's
velocity dispersion-size relationship, and constitute the first observational
evidence of a filament fully decoupled from the turbulent regime over
multi-parsec scales.Comment: 12 pages, 6 figures; Accepted for publication in A&
Unparticle inspired corrections to the Gravitational Quantum Well
We consider unparticle inspired corrections of the type
to the Newtonian potential in the context of the
gravitational quantum well. The new energy spectrum is computed and bounds on
the parameters of these corrections are obtained from the knowledge of the
energy eigenvalues of the gravitational quantum well as measured by the GRANIT
experiment.Comment: Revtex4 file, 4 pages, 2 figures and 1 table. Version to match the
one published at Physical Review
HP2 survey: III The California Molecular Cloud--A Sleeping Giant Revisited
We present new high resolution and dynamic range dust column density and
temperature maps of the California Molecular Cloud derived from a combination
of Planck and Herschel dust-emission maps, and 2MASS NIR dust-extinction maps.
We used these data to determine the ratio of the 2.2 micron extinction
coefficient to the 850 micron opacity and found the value to be close to that
found in similar studies of the Orion B and Perseus clouds but higher than that
characterizing the Orion A cloud, indicating that variations in the fundamental
optical properties of dust may exist between local clouds. We show that over a
wide range of extinction, the column density probability distribution function
(PDF) of the cloud can be well described by a simple power law with an
index that represents a steeper decline with column density than found in
similar studies of the Orion and Perseus clouds. Using only the protostellar
population of the cloud and our extinction maps we investigate the Schmidt
relation within the cloud. We show that the protostellar surface density,
, is directly proportional to the ratio of the protostellar and cloud
pdfs. We use the cumulative distribution of protostars to infer the functional
forms for both and PDF. We find that is best
described by two power-law functions with steeper indicies than found in other
local GMCs. We find that the protostellar pdf is a declining function of
extinction also best described by two power-laws whose behavior mirrors that of
. Our observations suggest that variations both in the slope of the
Schmidt relation and in the sizes of the protostellar populations between GMCs
are largely driven by variations in the slope of the cloud pdf. This confirms
earlier studies suggesting that cloud structure plays a major role in setting
the global star formation rates in GMCs.Comment: Accepted for publication in Astronomy and Astrophysics. Corrected
typos in source coordinates in table A.
Discontinuous operation promotes efficient continuous anaerobic treatment of effluents with high lipid content
A mixture of skim milk and sodium oleate was fed to an upflow sludge bed reactor
operated in cycles. Each cycle had a feeding phase under continuous operation and a reaction phase in
batch. Five cycles were performed with organic loading rates applied during feeding phases varying
between 4.4 and 8 kg COD.mˉ³.dˉ¹ and a constant hydraulic retention time of 1.6 days. In the first two
cycles, 70% of the methane-COD was produced in the reaction batch phase, whereas from the third to
the fifth cycles, biogas production in the reaction phase was less than 3% of total production. Overall
methane yields increased steadily, from 0.67 to 0.91 kg COD-CH4.kg COD removedˉ¹. LCFA
accumulated into the sludge in the first two cycles, being palmitate and stearate the dominant
intermediates quantified. In the subsequent cycles no LCFA were detected in the solid or liquid
phases. The specific methanogenic activity in the presence of acetate and H2/CO2 increased
significantly along the operation, particularly between time zero and the end of the third cycle. These
results show that a discontinuous operation promoted the development of an active anaerobic
community able to efficiently convert a continuous organic load of 8.2 kg COD.mˉ³.dˉ¹, from which
50% was oleate.European Commission - LIFE03 ENV/P/000501.Fundação para a Ciência e a Tecnologia (FCT) - POCTI/CTA/46328/2002
Fed-batch anaerobic degradation of long chain fatty acids
Efficient mineralization of effluents with high lipid content is possible in
anaerobic digesters when a sequential operation mode is applied, favoring the
adsorption of LCFA onto the sludge and then allowing the adsorbed substrate
to be biodegraded1-3. The study of adsorption along time can help to optimize
the process. Five batch assays were conducted in 160mL vials inoculated with
flocculent biomass and fed with sodium oleate (1g CQO/gVSS). Feeding was
applied during 10min (0.8ml/min), after which (t=0) a vial was immediately
sacrificed and analyzed for soluble COD, VSS and biomass-associated LCFA.
After 0.5, 1, 24 and 1000 hours of incubation at 37±1°C, 150rpm, one vial was
sacrificed and analyzed for the parameters stated before. Two additional vials
prepared and fed in a similar way and two blank controls (without substrate)
were incubated in the same conditions to follow cumulative methane
production. At the end of the feeding period, soluble COD removal efficiency
was 73%, corresponding exclusively to LCFA accumulation onto the sludge.
During the first 24 hours, methane or VFA production were negligible probably
due to residual substrate degradation. Palmitic acid accounted for 46 to 54% of
the biomass-associated LCFA and oleic acid for 31 to 40%. After 1000 hours of
incubation soluble COD removal was 86% and palmitic acid accounted for 100%
of the biomass-associated LCFA (45mg COD-LCFA/g VSS)
LCFA accumulation and biodegradation during anaerobic discontinuous treatment of an oleate-rich wastewater
The dynamics of medium and long-chain fatty acids (LCFA) accumulation and
biodegradation was studied during the anaerobic treatment of an oleate-rich wastewater. This
treatment was made in an upflow sludge bed reactor operated in cycles during 213 days. Five cycles
were performed, each one with a feeding phase in continuous and a reaction phase in batch. Saturated
and unsaturated fatty acids from C6 to C18 were extracted and analyzed by gas chromatography on
biomass samples collected at different key moments of the reactor operation. These biomass samples
were also incubated in batch assays and methane production from the accumulated substrate was
followed. LCFA accumulated onto the sludge during the first two cycles, reaching a maximum value
of 1.7 gCOD-LCFA.gVSˉ¹. Palmitate and stearate were the dominant intermediates quantified,
approximately in equal quantities. On the subsequent cycles only residual amounts of LCFA were
detected. Methane production on batch assays was higher than expected from the LCFA accumulated,
suggesting that other substrates could also be entrapped with the sludge. The results show that during
the first two cycles a specialized microbial consortium developed, able to treat oleate-rich
wastewaters.European Commission - LIFE03 ENV/P/000501.Fundação para a Ciência e a Tecnologia (FCT) - POCTI/CTA/46328/2002
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