394 research outputs found
Intense myocyte formation from cardiac stem cells in human cardiac hypertrophy
It is generally believed that increase in adult contractile cardiac mass can be accomplished only by hypertrophy of existing myocytes. Documentation of myocardial regeneration in acute stress has challenged this dogma and led to the proposition that myocyte renewal is fundamental to cardiac homeostasis. Here we report that in human aortic stenosis, increased cardiac mass results from a combination of myocyte hypertrophy and hyperplasia. Intense new myocyte formation results from the differentiation of stem-like cells committed to the myocyte lineage. These cells express stem cell markers and telomerase. Their number increased >13-fold in aortic stenosis. The finding of cell clusters with stem cells making the transition to cardiogenic and myocyte precursors, as well as very primitive myocytes that turn into terminally differentiated myocytes, provides a link between cardiac stem cells and myocyte differentiation. Growth and differentiation of these primitive cells was markedly enhanced in hypertrophy, consistent with activation of a restricted number of stem cells that, through symmetrical cell division, generate asynchronously differentiating progeny. These clusters strongly support the existence of cardiac stem cells that amplify and commit to the myocyte lineage in response to increased workload. Their presence is consistent with the notion that myocyte hyperplasia significantly contributes to cardiac hypertrophy and accounts for the subpopulation of cycling myocytes
Cardiac adaptations from 4 weeks of intensity-controlled vigorous exercise are lost after a similar period of detraining
Intensityâcontrolled (relative to VO2max) treadmill exercise training in adult rats results in the activation and ensuing differentiation of endogenous câkitpos cardiac stem/progenitor cells (eCSCs) into newly formed cardiomyocytes and capillaries. Whether these trainingâinduced adaptations persist following detraining is undetermined. Twelve male Wistar rats (~230 g) were exercised at 80â85% of their VO2max for 30 min dayâ1, 4 days weekâ1 for 4 weeks (TR; n = 6), followed by 4 weeks of detraining (DTR; n = 6). Twelve untrained rats acted as controls (CTRL). Exercise training significantly enhanced VO2max (11.34 mL kgâ1 minâ1) and wet heart weight (29%) above CTRL (P < 0.05). Echocardiography revealed that exercise training increased LV mass (~32%), posterior and septal wall thickness (~15%), ejection fraction and fractional shortening (~10%) compared to CTRL (P < 0.05). Cardiomyocyte diameter (17.9 ± 0.1 ÎŒm vs. 14.9 ± 0.6 ÎŒm), newly formed (BrdUpos/Ki67pos) cardiomyocytes (7.2 ± 1.3%/1.9 ± 0.7% vs. 0.2 ± 0.1%/0.1 ± 0.1%), total cardiomyocyte number (45.6 ± 0.6 Ă 106 vs. 42.5 ± 0.4 Ă 106), câkitpos eCSC number (884 ± 112 per 106 cardiomyocytes vs. 482 ± 132 per 106 cardiomyocytes), and capillary density (4123 ± 227 per mm2 vs. 2117 ± 118 per mm2) were significantly greater in the LV of trained animals (P < 0.05) than CTRL. Detraining removed the stimulus for câkitpos eCSC activation (640 ± 98 per 106 cardiomyocytes) and resultant cardiomyocyte hyperplasia (0.4 ± 0.3% BrdUpos/0.2 ± 0.2% Ki67pos cardiomyocytes). Capillary density (3673 ± 374 per mm2) and total myocyte number (44.7 ± 0.5 Ă 106) remained elevated following detraining, but cardiomyocyte hypertrophy (15.0 ± 0.4 ÎŒm) was lost, resulting in a reduction of anatomical (wall thickness ~4%; LV mass ~10% and cardiac mass ~8%, above CTRL) and functional (EF & FS ~2% above CTRL) parameters gained through exercise training. These findings demonstrate that cardiac adaptations, produced by 4 weeks of intensityâcontrolled exercise training are lost after a similar period of detraining
Large Eddy simulations of isolated and installed jet noise using the high-order discontinuous Galerkin method
A recently developed computational framework for jet noise is used to compute the noise generated by an isolated and installed jet. The framework consists of two parts. In the first part, the spectral/hp element framework Nektar++ is used to compute the near-field flow. Nektar++ solves the unfiltered Navier-Stokes equations on unstructured grids using the high-order discontinuous Galerkin method. The discrete equations are integrated in time using an implicit scheme based on the matrix-free Newton-GMRES method. In the second part, the Antares library is used to compute the far-field noise. Antares solves the Ffowcs Williams - Hawkings equation for a permeable integration surface in the time domain using a source-time dominant algorithm. The simulations are validated against experimental data obtained in the Doak Laboratory Flight Jet Rig, located at the University of Southampton. For the isolated jet, good agreement is achieved, both in terms of the flow statistics and the far-field noise. The discrepancies observed for the isolated jet are believed to be caused by an under-resolved boundary layer in the simulations. For the installed jet, the flow statistics are also well predicted. In the far-field, very good agreement is achieved for downstream observers. For upstream observers, some discrepancies are observed for very high and very low frequencies
The adult heart responds to increased workload with physiologic hypertrophy, cardiac stem cell activation, and new myocyte formation
Aims It is a dogma of cardiovascular pathophysiology that the increased cardiac mass in response to increased workload is produced by the hypertrophy of the pre-existing myocytes. The role, if any, of adult-resident endogenous cardiac stem/progenitor cells (eCSCs) and new cardiomyocyte formation in physiological cardiac remodelling remains unexplored. Methods and results In response to regular, intensity-controlled exercise training, adult rats respond with hypertrophy of the pre-existing myocytes. In addition, a significant number (âŒ7%) of smaller newly formed BrdU-positive cardiomyocytes are produced by the exercised animals. Capillary density significantly increased in exercised animals, balancing cardiomyogenesis with neo-angiogenesis. c-kitpos eCSCs increased their number and activated state in exercising vs. sedentary animals. c-kitpos eCSCs in exercised hearts showed an increased expression of transcription factors, indicative of their commitment to either the cardiomyocyte (Nkx2.5pos) or capillary (Ets-1pos) lineages. These adaptations were dependent on exercise duration and intensity. Insulin-like growth factor-1, transforming growth factor-ÎČ1, neuregulin-1, bone morphogenetic protein-10, and periostin were significantly up-regulated in cardiomyocytes of exercised vs. sedentary animals. These factors differentially stimulated c-kitpos eCSC proliferation and commitment in vitro, pointing to a similar role in vivo. Conclusion Intensity-controlled exercise training initiates myocardial remodelling through increased cardiomyocyte growth factor expression leading to cardiomyocyte hypertrophy and to activation and ensuing differentiation of c-kitpos eCSCs. This leads to the generation of new myocardial cells. These findings highlight the endogenous regenerative capacity of the adult heart, represented by the eCSCs, and the fact that the physiological cardiac adaptation to exercise stress is a combination of cardiomyocyte hypertrophy and hyperplasia (cardiomyocytes and capillaries)
Deuteration around the ultracompact HII region Mon R2
The massive star-forming region Mon R2 hosts the closest ultra-compact HII
region that can be spatially resolved with current single-dish telescopes. We
used the IRAM-30m telescope to carry out an unbiased spectral survey toward two
important positions (namely IF and MP2), in order to studying the chemistry of
deuterated molecules toward Mon R2. We found a rich chemistry of deuterated
species at both positions, with detections of C2D, DCN, DNC, DCO+, D2CO, HDCO,
NH2D, and N2D+ and their corresponding hydrogenated species and isotopologs.
Our high spectral resolution observations allowed us to resolve three velocity
components: the component at 10 km/s is detected at both positions and seems
associated with the layer most exposed to the UV radiation from IRS 1; the
component at 12 km/s is found toward the IF position and seems related to the
molecular gas; finally, a component at 8.5 km/s is only detected toward the MP2
position, most likely related to a low-UV irradiated PDR. We derived the column
density of all the species, and determined the deuterium fractions (Dfrac). The
values of Dfrac are around 0.01 for all the observed species, except for HCO+
and N2H+ which have values 10 times lower. The values found in Mon R2 are well
explained with pseudo-time-dependent gas-phase model in which deuteration
occurs mainly via ion-molecule reactions with H2D+, CH2D+ and C2HD+. Finally,
the [H13CN]/[HN13C] ratio is very high (~11) for the 10 km/s component, which
also agree with our model predictions for an age of ~0.01-0.1 Myr. The
deuterium chemistry is a good tool for studying star-forming regions. The
low-mass star-forming regions seem well characterized with Dfrac(N2H+) or
Dfrac(HCO+), but it is required a complete chemical modeling to date massive
star-forming regions, because the higher gas temperature together with the
rapid evolution of massive protostars.Comment: 14 pages of manuscript, 17 pages of apendix, 7 figures in the main
text, accepted for publication in A&
P365Protection against doxorubicine-induced cardiomyopathy by bergamot polyphenols through myocyte survival and cardiac stem cell activation
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Unraveling UBC 274: a morphological, kinematical and chemical analysis of a disrupting open cluster
We do a morphological, kinematic and chemical analysis of the disrupting
cluster UBC 274 (2.5 Gyr, pc) to study its global properties. We use
HDBSCAN to obtain a new membership list up to 50 pc from its centre and up to
magnitude using Gaia EDR3 data. We use high resolution and high
signal-to-noise spectra to obtain atmospheric parameters of 6 giants and
subgiants, and individual abundances of 18 chemical species. The cluster has a
highly eccentric (0.93) component, tilted 10 deg with respect to the
plane of the Galaxy, which is morphologically compatible with the result of a
test-particle simulation of a disrupting cluster. Our abundance analysis shows
that the cluster has a subsolar metallicity of [Fe/H]. Its
chemical pattern is compatible with that of Ruprecht 147, of similar age but
located closer to the Sun, with the remarkable exception of neutron-capture
elements, which present an overabundance of . The
cluster's elongated morphology is associated with the internal part of its
tidal tail, following the expected dynamical process of disruption. We find a
significant sign of mass segregation where the most massive stars appear 1.5
times more concentrated than other stars. The cluster's overabundance of
neutron-capture elements can be related to the metallicity dependence of the
neutron-capture yields due to the secondary nature of these elements, predicted
by some models. UBC 274 presents a high chemical homogeneity at the level of
dex in the sampled region of its tidal tails.Comment: Accepted by A&
Aeroacoustic analysis of a closely installed chevron nozzle jet using the high-order discontinuous Galerkin method
In this paper, we use Large Eddy Simulations (LES) in combination with the Ffowcs Williams - Hawkings method to study the influence of chevrons on the flow field as well as the noise produced by a closely installed M = 0.6 jet. The LES simulations are performed with the spectral/hp element framework Nektar++. Nektar++ uses the high-order discontinuous Galerkin method and an implicit scheme based on the matrix-free Newton-GMRES method to discretize the unfiltered Navier-Stokes equations in space and time, respectively. The far-field noise is computed using Antares. Antares solves the Ffowcs Williams - Hawkings equation for a permeable integration surface in the time-domain using a source-time dominant algorithm. The aerodynamic results show good agreement with experimental data obtained in the Doak Laboratory Flight Jet Rig, located at the University of Southampton. Some discrepancies are observed in terms of the far-field noise levels, especially for higher polar observer angles relative to the downstream jet axis. In terms of noise reduction potential, the simulations predict that the chevrons reduce the OASPL by 1dB compared to an installed round nozzle for all observers located on the unshielded side of the wing. This should be compared to the experiments, which predict a 1.5dB noise reduction for the same chevron nozzle
Massive young disks around Herbig Ae stars
Herbig Ae stars (HAe) are the precursors of Vega-type systems and, therefore,
crucial objects in planet formation studies. Thus far, only a few disks
associated with HAe stars have been studied using millimetre interferometers.
Our aim is to determine the dust evolution and the lifetime of the disks
associated with Herbig Ae stars. We imaged the continuum emission at 3 mm and
1.3 mm of the Herbig Ae/Be stars BD+61154, RR Tau, VY Mon and LkHa 198 using
the Plateau de Bure Interferometer (PdBI). These stars are in the upper end of
the stellar mass range of the Herbig Ae stars (stellar mass greater than 3
solar masses). Our measurements were used to complete the Spectral Energy
Distribution (SED). The modelling of the SED, in particular the FIR-mm part,
allow us to determine the masses and dust properties of these disks. We
detected the disks associated with BD+61154, RR Tau and VY Mon with disk masses
of 0.35 Msun, 0.05 Msun and 0.40 Msun respectively. The disk around LkHa 198
was not detected with an upper limit to the disk mass of 0.004 Msun. We
detected, however, the disks associated with the younger stellar objects LkHa
198--IR and LkHa 198-mm that are located in the vicinity of LkHa 198. The
fitting of the mm part of the SED reveal that the grains in the mid-plane of
the disks around BD+61154, RR Tau and VY Mon have sizes of 1--1000 microns.
Therefore, grains have not grown to centimetre sizes in these disks yet. These
massive (M>3 Msun) and young (about 1 Myr) HAe stars are surrounded by massive
(>0.04 Msun) disks with grains of micron-millimetre sizes. Although grain
growth is proceeding in these disks, their evolutionary stage is prior to the
formation of planetesimals. These disks are less evolved than those detected
around T Tauri and Herbig Be stars
Bone marrow cells differentiate in cardiac cell lineages after infarction independently of cell fusion.
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