85 research outputs found
Red Giant stars in the Large Magellanic Cloud clusters
We present deep J,H,Ks photometry and accurate Color Magnitude Diagrams down
to K ~18.5, for a sample of 13 globular clusters in the Large Magellanic Cloud.
This data set combined with the previous sample of 6 clusters published by our
group gives the opportunity to study the properties of giant stars in clusters
with different ages (ranging from ~80 Myr up to ~3.5 Gyr). Quantitative
estimates of star population ratios (by number and luminosity) in the
Asymptotic Giant Branch, the Red Giant Branch and the He-clump, have been
obtained and compared with theoretical models in the framework of probing the
so-called phase transitions. The AGB contribution to the total luminosity
starts to be significant at ~200 Myr and reaches its maximum at ~5-600 Myr,
when the RGB Phase Transition is starting. At ~900 Myr the full developing of
an extended and well populated RGB has been completed. Both the occurrence of
the AGB and RGB Phase Transitions are sharp events, lasting a few hundreds Myr
only. These empirical results agree very well with the theoretical predictions
of simple stellar population models based on canonical tracks and the
fuel-consumption approach.Comment: 32 pages, 11 figures, accepted to Ap
The Herbal Drug Melampyrum pratense
Melampyrum pratense L. (Koch) is used in traditional Austrian medicine for the treatment of different inflammation-related conditions.
In this work, we show that the extracts of M. pratense stimulated peroxisome proliferator-activated receptors- (PPARs-)α
and -γ that are well recognized for their anti-inflammatory activities. Furthermore, the extract inhibited the activation of the proinflammatory transcription
factor NF-κB and induction of its target genes interleukin-8 (IL-8) and E-selectin in vitro. Bioassay-guided fractionation
identified several active flavonoids and iridoids including melampyroside and mussaenoside and the phenolic compound lunularin that were identified in this
species for the first time. The flavonoids apigenin and luteolin were distinguished as the main components accountable for the anti-inflammatory properties.
Apigenin and luteolin effectively inhibited tumor necrosis factor α (TNF-α)-induced NF-κB-mediated transactivation of a luciferase reporter gene.
Furthermore, the two compounds dose-dependently reduced IL-8 and E-selectin protein expression after stimulation with lipopolysaccharide (LPS) or TNF-α in endothelial cells (ECs).
The iridoids melampyroside and mussaenoside prevented the elevation of E-selectin in LPS-stimulated ECs. Lunularin was found to reduce the protein levels
of the proinflammatory mediators E-selectin and IL-8 in ECs in response to LPS. These data validate the ethnomedical use of M. pratense for the treatment
of inflammatory conditions and point to the constituents accountable for its anti-inflammatory activity
The globular cluster system of NGC 1399. III. VLT spectroscopy and database
Radial velocities of 468 globular clusters around NGC 1399, the central galaxy in the Fornax cluster, have been obtained with FORS2 and the Mask Exchange Unit (MXU) at the ESO Very Large Telescope. This is the largest sample of globular cluster velocities around any galaxy obtained so far. The mean velocity uncertainty is 50 km s-1. This data sample is accurate and large enough to be used in studies of the mass distribution of NGC 1399 and the properties of its globular cluster system. Here we describe the observations and the reduction procedure, and we discuss the uncertainties of the resulting velocities. The complete sample of cluster velocities that is used in a dynamical study of NGC 1399 is tabulated. A subsample is compared with previously published values.Facultad de Ciencias Astronómicas y Geofísica
A Database of 2MASS Near-Infrared Colors of Magellanic Cloud Star Clusters
The (rest-frame) near-IR domain contains important stellar population
diagnostics and is often used to estimate masses of galaxies at low as well as
high redshifts. However, many stellar population models are still relatively
poorly calibrated in this part of the spectrum. To allow an improvement of this
calibration we present a new database of integrated near-infrared JHKs
magnitudes for 75 star clusters in the Magellanic Clouds, using the 2-Micron
All-Sky Survey (2MASS). The majority of the clusters in our sample have robust
age and metallicity estimates from color-magnitude diagrams available in the
literature, and populate a range of ages from 10 Myr to 15 Gyr and a range in
[Fe/H] from -2.17 to +0.01 dex. A comparison with matched star clusters in the
2MASS Extended Source Catalog (XSC) reveals that the XSC only provides a good
fit to the unresolved component of the cluster stellar population. We also
compare our results with the often-cited single-channel JHK photometry of
Persson and collaborators, and find significant differences, especially for
their 30"-diameter apertures up to ~2.5 mag in the K-band, more than 1 mag in
J-K, and up to 0.5 mag in H-K. Using simulations to center apertures based on
maximum light throughput (as performed by Persson et al, we show that these
differences can be attributed to near-IR-bright cluster stars (e.g., Carbon
stars) located away from the true center of the star clusters. The wide age and
metallicity coverage of our integrated JHKs photometry sample constitutes a
fundamental dataset for testing population synthesis model predictions, and for
direct comparison with near-IR observations of distant stellar populations.Comment: AJ August 2006 issue, 67 pages, 8 tables, 17 figure
The Chemical Enrichment History of the Large Magellanic Cloud
Ca II triplet spectroscopy has been used to derive stellar metallicities for
individual stars in four LMC fields situated at galactocentric distances of
3\arcdeg, 5\arcdeg, 6\arcdeg\@ and 8\arcdeg\@ to the north of the Bar. Observed
metallicity distributions show a well defined peak, with a tail toward low
metallicities. The mean metallicity remains constant until 6\arcdeg\@
([Fe/H]-0.5 dex), while for the outermost field, at 8\arcdeg, the mean
metallicity is substantially lower than in the rest of the disk
([Fe/H]-0.8 dex). The combination of spectroscopy with deep CCD
photometry has allowed us to break the RGB age--metallicity degeneracy and
compute the ages for the objects observed spectroscopically. The obtained
age--metallicity relationships for our four fields are statistically
indistinguishable. We conclude that the lower mean metallicity in the outermost
field is a consequence of it having a lower fraction of intermediate-age stars,
which are more metal-rich than the older stars. The disk age--metallicity
relationship is similar to that for clusters. However, the lack of objects with
ages between 3 and 10 Gyr is not observed in the field population. Finally, we
used data from the literature to derive consistently the age--metallicity
relationship of the bar. Simple chemical evolution models have been used to
reproduce the observed age--metallicity relationships with the purpose of
investigating which mechanism has participated in the evolution of the disk and
bar. We find that while the disk age--metallicity relationship is well
reproduced by close-box models or models with a small degree of outflow, that
of the bar is only reproduced by models with combination of infall and outflow.Comment: 45 pages, 10 figures, accepted for publication in Astronomical
Journa
The globular cluster system of NGC 1399. III. VLT spectroscopy and database
Radial velocities of 468 globular clusters around NGC 1399, the central galaxy in the Fornax cluster, have been obtained with FORS2 and the Mask Exchange Unit (MXU) at the ESO Very Large Telescope. This is the largest sample of globular cluster velocities around any galaxy obtained so far. The mean velocity uncertainty is 50 km s-1. This data sample is accurate and large enough to be used in studies of the mass distribution of NGC 1399 and the properties of its globular cluster system. Here we describe the observations and the reduction procedure, and we discuss the uncertainties of the resulting velocities. The complete sample of cluster velocities that is used in a dynamical study of NGC 1399 is tabulated. A subsample is compared with previously published values.Facultad de Ciencias Astronómicas y Geofísica
The globular cluster NGC 1978 in the Large Magellanic Cloud
We have used deep high-resolution Hubble Space Telescope ACS observations to
image the cluster NGC 1978 in the Large Magellanic Cloud. This high-quality
photometric data set allowed us to confirm the high ellipticity (~0.30+-0.02)
of this stellar system. The derived Color Magnitude Diagram allowed a detailed
study of the main evolutionary sequences: in particular we have detected the so
called Bump along the Red Giant Branch (at V_{555}=19.10+-0.10). This is the
first detection of this feature in an intermediate-age cluster. Moreover the
morphology of the evolutionary sequence and their population ratios have been
compared with the expectations of different theoretical models (namely BaSTI,
PEL and Padua) in order to quantify the effect of convective overshooting. The
best agreement (both in terms of morphology and star counts) has been found the
PEL (Pisa Evolutionary Library) isochrone with Z=0.008 (consistenly with the
most recent determination of the cluster metallicity, [M/H]=-0.37 dex) and a
mild overshooting efficiency (Lambda_{os}=0.1). By adopting this theoretical
set an age of 1.9+-0.1 Gyr has been obtained.Comment: 26 pages, 8 figures, accepted to A
The Globular Cluster System of NGC 1399. II. Kinematics of a Large Sample of Globular Clusters
We study the kinematics and dynamics of the globular cluster system of NGC
1399, the central galaxy of the Fornax cluster. The observational data consists
of medium resolution spectra, obtained at the Very Large Telescope. Our sample
comprises 468 radial velocities in the magnitude range 20 < m_R < 23. This is
the largest sample of globular cluster velocities around any galaxy obtained so
far. The radial range is 2 arcmin < r < 9 arcmin, corresponding to 11 kpc to 50
kpc of galactocentric distance. There is the possibility that unbound clusters
and/or objects in the foreground contaminate the NGC 1399 cluster sample. Under
strong error selection, practically no objects are found with velocities lower
than 800 km/s or higher than 2000 km/s. Since the extreme velocities influence
the velocity dispersion considerably, uncertainty regarding the exact value of
the dispersion remains. Within the above velocity limits, we derive a projected
velocity dispersion for the total sample of 274+-9 km/s which within the
uncertainties remains constant over the entire radial range. Without any
velocity restriction, it increases to 325 km/s. Blue and red clusters show
different dispersions corresponding to their different surface density
profiles. Spherical models point to a circular velocity of 415+-30$ km/s,
assuming isotropy for the red clusters. This value is constant out to 40 kpc.
The inferred dark halo potential can be well represented by a logarithmic
potential. Also a halo of the NFW type fits well to the observations. Some mass
profiles derived from X-ray analyses do not agree with a constant circular
velocity within our radial range, irrespective of its exact value.Comment: 38 pages, 20 figures, accepted by A
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