44 research outputs found
Effects of the environment on galaxies in the Catalogue of Isolated Galaxies: physical satellites and large scale structure
We aim to identify and quantify the effects of the satellite distribution
around a sample of galaxies in the Catalogue of Isolated Galaxies (CIG), as
well as the effects of the Large Scale Structure (LSS) using the SDSS-DR9. To
recover the physically bound galaxies we focus on the satellites which are
within the escape speed of each CIG galaxy. We also propose a more conservative
method using the stacked Gaussian distribution of the velocity difference of
the neighbours. The tidal strengths affecting the primary galaxy are estimated
to quantify the effects of the local and LSS environments. We also define the
projected number density parameter at the 5 nearest neighbour to
characterise the LSS around the CIG galaxies. Out of the 386 CIG galaxies
considered in this study, at least 340 (88\% of the sample) have no physically
linked satellite. Out of the 386 CIG galaxies, 327 (85\% of the sample) have no
physical companion within a projected distance of 0.3 Mpc. The CIG galaxies are
distributed following the LSS of the local Universe, although presenting a
large heterogeneity in their degree of connection with it. A clear segregation
appears between early-type CIG galaxies with companions and isolated late-type
CIG galaxies. Isolated galaxies are in general bluer, with likely younger
stellar populations and rather high star formation with respect to older,
redder CIG galaxies with companions. Reciprocally, the satellites are redder
and with an older stellar populations around massive early-type CIG galaxies,
while they have a younger stellar content around massive late-type CIG
galaxies. This suggests that the CIG is composed of a heterogeneous population
of galaxies, sampling from old to more recent, dynamical systems of galaxies.Comment: 19 pages, 10 figures, 1 table, accepted for publication in Astronomy
& Astrophysic
A permeability-increasing drug synergizes with bacterial efux pump inhibitors and restores susceptibility to antibiotics in multi-drug resistant Pseudomonas aeruginosa strains
Resistance to antibiotics poses a major global threat according to the World Health Organization. Restoring the activity of existing drugs is an attractive alternative to address this challenge. One of the most efficient mechanisms of bacterial resistance involves the expression of efflux pump systems capable of expelling antibiotics from the cell. Although there are efflux pump inhibitors (EPIs) available, these molecules are toxic for humans. We hypothesized that permeability-increasing antimicrobial peptides (AMPs) could lower the amount of EPI necessary to sensitize bacteria to antibiotics that are efflux substrates. To test this hypothesis, we measured the ability of polymyxin B nonapeptide (PMBN), to synergize with antibiotics in the presence of EPIs. Assays were performed using planktonic and biofilm-forming cells of Pseudomonas aeruginosa strains overexpressing the MexAB-OprM efflux system. Synergy between PMBN and EPIs boosted azithromycin activity by a factor of 2,133 and sensitized P. aeruginosa to all tested antibiotics. This reduced several orders of magnitude the amount of inhibitor needed for antibiotic sensitization. The selected antibiotic-EPI-PMBN combination caused a 10 million-fold reduction in the viability of biofilm forming cells. We proved that AMPs can synergize with EPIs and that this phenomenon can be exploited to sensitize bacteria to antibiotics
The AMIGA sample of isolated galaxies XI. A First Look at Isolated Galaxy Colors
The basic properties of galaxies can be affected by both nature (internal
processes) or nurture (interactions and effects of environment). Deconvolving
the two effects is an important current effort in astrophysics. Observed
properties of a sample of isolated galaxies should be largely the result of
internal (natural) evolution. It follows that nurture-induced galaxy evolution
can only be understood through comparative study of galaxies in different
environments. We take a first look at SDSS (g-r) colors of galaxies in the
AMIGA sample involving many of the most isolated galaxies in the local
Universe. This leads us to simultaneously consider the pitfalls of using
automated SDSS colors. We focus on median values for the principal
morphological subtypes found in the AMIGA sample (E/S0 and Sb-Sc) and compare
them with equivalent measures obtained for galaxies in denser environments. We
find a weak tendency for AMIGA spiral galaxies to be redder than objects in
close pairs. We find no clear difference when we compare with galaxies in other
(e.g. group) environments. However, the (g-r) color of isolated galaxies shows
a Gaussian distribution as might be expected assuming nurture-free evolution.
We find a smaller median absolute deviation in colors for isolated galaxies
compared to both wide and close pairs. The majority of the deviation on median
colors for spiral subtypes is caused by a color-luminosity correlation.
Surprisingly isolated and non-isolated early-type galaxies show similar (g-r).
We see little evidence for a green valley in our sample with most spirals
redder than (g-r)=0.7 having spurious colors. The redder colors of AMIGA
spirals and lower color dispersions for AMIGA subtypes -compared with close
pairs- is likely due to a more passive star formation in very isolated
galaxies.Comment: Accepted for publication in A&A. 9 pages, 7 Figures, and 2 tables,
one only available onlin
Unveiling the environment and faint features of the isolated galaxy CIG 96 with deep optical and HI observations
Asymmetries in HI in galaxies are often caused by the interaction with close
companions, making isolated galaxies an ideal framework to study secular
evolution. The AMIGA project has demonstrated that isolated galaxies show the
lowest level of asymmetry in their HI integrated profiles, yet some present
significant asymmetries. CIG 96 (NGC 864) is a representative case reaching a
16% level. Our aim is to investigate the HI asymmetries of this spiral galaxy
and what processes have triggered the star-forming regions observed in the XUV
pseudoring. We performed deep optical observations at CAHA 1.23m, 2.2m and VST
telescopes. We reach surface brightness (SB) limits of mu_2.2m = 27.5 mag
arcsec-2 (Cous R) and mu_VST = 28.7mag arcsec-2 (r) that show the XUV
pseudoring of the galaxy in detail. Additionally, a wavelet filtering of the HI
data cube from our deep observations with E/VLA telescope allowed us to reach a
column density of N_HI = 8.9x10^18 cm -2 (5sigma) (28"x28" beam), lower than in
any isolated galaxy. We confirm that the HI extends farther than 4xr_25 in all
directions. Furthermore, we detect for the first time two gaseous structures
(10^6 Msol) in the outskirts. The g-r colour index image from 1.23m shows
extremely blue colours in certain regions of the pseudoring where
N_HI>8.5x10^20 cm-2 , whereas the rest show red colours. Galactic cirrus
contaminate the field, setting an unavoidable detection limit at 28.5mag
arcsec-2 (r). We detect no stellar link within 1degx1deg or gaseous link within
40'x40' between CIG 96 and any companion. The isolation criteria rule out
interactions with other similar-sized galaxies for at least 2.7Gyr. Using
existing stellar evolution models, the age of the pseudoring is estimated at
1Gyr or older. Undetected previously accreted companions and cold gas accretion
remain as the main hypothesis to explain the optical pseudoring and HI features
of CIG 96.Comment: 23 pages, 18 figures, 4 table
Effectiveness of the Epley’s maneuver performed in primary care to treat posterior canal benign paroxysmal positional vertigo: study protocol for a randomized controlled trial
Factors affecting the establishment of the invasive crayfish Procambarus clarkii (Crustacea, Decapoda) in the Mediterranean rivers of the northeastern Iberian Peninsula
It is essential to find the combination of factors associated with ecosystem invasibility, as this forms part of basic knowledge on biological invasions and provides important information to guide management and conservation decisions. We surveyed 325 sampling sites in Catalonia to investigate relationships between crayfish presence and a series of biotic and abiotic factors, including fish abundance and species richness, geographical features, and water mineralization and eutrophication. Abiotic data provided by 29 environmental variables were studied by principal-components analysis. We then used a combination of three statistical approaches (comparison of average scores, general linear mixed models, and hierarchical partitioning analysis) to determine the potential relationship between crayfish occurrence and predictors. Our findings seem to indicate that the presence of crayfish was associated with geographical features, water mineralization and eutrophication, and the introduction of non-indigenous fish species to Catalonia. Our results also suggest that re-establishment of the natural hydrology of Mediterranean streams could hinder the spread of Procambarus clarkii. This, combined with preservation of headwater streams and attempts at local extirpation of P. clarkii, would favour native species and, potentially, enable the successful reintroduction of the native white-clawed crayfish (Austropotamobius pallipes species complex)
Potenciación de antibióticos, inhibidores de betalactamasas y bombas de expulsión mediante péptidos antimicrobianos en bacterias gramnegativas multiresistentes
Resistance to antibiotics poses a “major global threat” to public health according to
World Health Organization. The increasing emergence of bacterial clones insensitive to
these drugs greatly limits the therapeutic options for infectious diseases and highlights
the urgent need to develop novel treatments effective against these organisms. In the
present work, we demonstrated that subinhibitory concentrations of certain antimicrobial
peptides can neutralize several antibiotic resistance mechanisms expressed by Gramnegative
multi-drug resistant pathogens such as Klebsiella pneumoniae and
Pseudomonas aeruginosa (“ESKAPE” pathogens) and Escherichia coli. This
enhancement of antibiotic activity resulted in the sensitization of these organisms to
several antibiotic classes.
We hypothesized that antimicrobial peptides could potentiate the activity of inhibitors
of either β-lactamases or antibiotic efflux pump systems and sensitize bacteria to
antibiotics substrate of those resistance mechanisms. To test this hypothesis we
measured the ability of peptides to synergize with those antibiotics in the presence of
selected inhibitors of those systems. As peptides, we used the nonapeptides of
polymyxin B and polymyxin E (PMBN and PMEN), as well as a peptide library derived
from human lactoferricin with improved bacterial permeabilizing activity and very low
toxicity towards human cells. To characterize the antimicrobial efficiency of the
combinations, we used an array of techniques including conventional MIC/MBC testing,
checkerboard analysis, growth kinetics, killing curves, and anti-biofilm activity against
biofilms measured by confocal microscopy and viable counts on biofilms grown under
static (on microplates) and dynamic (in a CDC-reactor) flow regimes. Using planktonic
cultures, we demonstrated that, PMBN was able to greatly enhance the activity of
several (i) β-lactamase inhibitors in a β-lactamase AmpC overproducing P. aeruginosa
strain (potentiating the activity of amoxicillin, ampicillin, ticarcillin, piperacillin and
ceftazidime), (ii) β-lactamase inhibitors in ESBL-producing Enterobacteriaceae strains
(sensitizing them to ampicillin, amoxicillin, ticarcillin and piperacillin) and (iii) efflux pump
inhibitors in a MexAB-OprM pump P. aeruginosa overproducing strain (enhancing the
activity of aztreonam, ceftazidime, doxycycline, levofloxacin, piperacillin and
azithromycin). In addition, all the triple combinations selected were able to cause a 10-
100 million fold reduction in the viability of biofilm forming cells.
Finally, we showed that these antimicrobial peptides can potentiate not only
resistance mechanism inhibitors (β-lactamases and efflux pumps), but they can also
enhance the activity of several antibiotics that specifically target Gram-positive bacteria
(i.e. vancomycin), sensitizing P. aeruginosa, E. coli and K. pneumoniae to them. This strategy allows the use of these combinations as empirical therapy with a broad
spectrum of activity
Potenciación de antibióticos, inhibidores de betalactamasas y bombas de expulsión mediante péptidos antimicrobianos en bacterias gramnegativas multiresistentes
Resistance to antibiotics poses a “major global threat” to public health according to
World Health Organization. The increasing emergence of bacterial clones insensitive to
these drugs greatly limits the therapeutic options for infectious diseases and highlights
the urgent need to develop novel treatments effective against these organisms. In the
present work, we demonstrated that subinhibitory concentrations of certain antimicrobial
peptides can neutralize several antibiotic resistance mechanisms expressed by Gramnegative
multi-drug resistant pathogens such as Klebsiella pneumoniae and
Pseudomonas aeruginosa (“ESKAPE” pathogens) and Escherichia coli. This
enhancement of antibiotic activity resulted in the sensitization of these organisms to
several antibiotic classes.
We hypothesized that antimicrobial peptides could potentiate the activity of inhibitors
of either β-lactamases or antibiotic efflux pump systems and sensitize bacteria to
antibiotics substrate of those resistance mechanisms. To test this hypothesis we
measured the ability of peptides to synergize with those antibiotics in the presence of
selected inhibitors of those systems. As peptides, we used the nonapeptides of
polymyxin B and polymyxin E (PMBN and PMEN), as well as a peptide library derived
from human lactoferricin with improved bacterial permeabilizing activity and very low
toxicity towards human cells. To characterize the antimicrobial efficiency of the
combinations, we used an array of techniques including conventional MIC/MBC testing,
checkerboard analysis, growth kinetics, killing curves, and anti-biofilm activity against
biofilms measured by confocal microscopy and viable counts on biofilms grown under
static (on microplates) and dynamic (in a CDC-reactor) flow regimes. Using planktonic
cultures, we demonstrated that, PMBN was able to greatly enhance the activity of
several (i) β-lactamase inhibitors in a β-lactamase AmpC overproducing P. aeruginosa
strain (potentiating the activity of amoxicillin, ampicillin, ticarcillin, piperacillin and
ceftazidime), (ii) β-lactamase inhibitors in ESBL-producing Enterobacteriaceae strains
(sensitizing them to ampicillin, amoxicillin, ticarcillin and piperacillin) and (iii) efflux pump
inhibitors in a MexAB-OprM pump P. aeruginosa overproducing strain (enhancing the
activity of aztreonam, ceftazidime, doxycycline, levofloxacin, piperacillin and
azithromycin). In addition, all the triple combinations selected were able to cause a 10-
100 million fold reduction in the viability of biofilm forming cells.
Finally, we showed that these antimicrobial peptides can potentiate not only
resistance mechanism inhibitors (β-lactamases and efflux pumps), but they can also
enhance the activity of several antibiotics that specifically target Gram-positive bacteria
(i.e. vancomycin), sensitizing P. aeruginosa, E. coli and K. pneumoniae to them. This strategy allows the use of these combinations as empirical therapy with a broad
spectrum of activity