178 research outputs found
The surface brightness profile of the remote cluster NGC 2419
It is well known that the bright and remote Galactic globular cluster NGC2419
has a very peculiar structure. In particular its half-light radius is
significantly larger than that of ordinary globular clusters of similar
luminosity, being as large as that of the brightest nuclei of dwarf elliptical
galaxies. In this context it is particularly worth to check the reliability of
the existing surface brightness profiles for this cluster and of the available
estimates of its structural parameters. Combining different datasets I derive
the surface brightness profile going from the cluster center out to ~ 480
arcsec, i.e. ~25 core radii. (Abridged). The newly obtained surface brightness
profile is in excellent agreement with that provided by Trager, King &
Djorgovski for r>= 4 arcsec; it is best fitted by a King model having r_c=0.32
arcmin, mu_V(0)=19.55 and C=1.35. Also new independent estimates of the total
integrated V magnitude (V_t=10.47 +/- 0.07) and of the half-light radius
(r_h=0.96 arcmin +/- 0.2 arcmin) have been obtained. (Abridged). The structure
of NGC2419 is now reliably constrained by (at least) two fully independent
observational profiles that are in good agreement one with the other. Also the
overall agreement between structural parameters independently obtained by
different authors is quite satisfying.Comment: Research Note, accepted for publication by A&A. 6 pages with 4
figures + 3 pages of Online Material (table
The Sagittarius Dwarf spheroidal Galaxy Survey (SDGS) II: The stellar content and constraints on the star formation history
A detailed study of the Star Formation History of the Sgr dSph galaxy is
performed through the analysis of the data from the Sagittarius Dwarf Galaxy
Survey (SDGS; Bellazzini, Ferraro & Buonanno 1999). Accurate statistical
decontamination of the SDGS Color - Magnitude diagrams allow us to obtain many
useful constraints on the age and metal content of the Sgr stellar populations
in three different region of the galaxy.
A coarse metallicity distribution of Sgr stars is derived, ranging from
[Fe/H]~ -2.0 to [Fe/H]~ -0.7, the upper limit being somewhat higher in the
central region of the galaxy. A qualitative global fit to all the observed CMD
features is attempted, and a general scheme for the Star Formation History of
the Sgr is derived. According to this scheme, star formation began at very
early time from a low metal content Inter Stellar Medium and lasted for several
Gyr, coupled with progressive chemical enrichment. The Star Formation Rate
(SFR) had a peak from 8 to 10 gyr ago when the mean metallicity was in the
range -1.3<= [Fe/H] <= -0.7. After that maximum, the SFR rapidly decreased and
very low rate star formation took place until ~1-0.5 Gyr ago.Comment: 21 pages, 12 figures, figg. 1,2,3,5,6,10 and 11 provided in lower
resolution format. For full resolution versions see
http://www.bo.astro.it/bap/BAPhome.html Accepted by MNRA
Chemical enrichment in very low-metallicity environments: Bootes I
We present different chemical evolution models for the ultrafaint dwarf
galaxy Bootes I. We either assume that the galaxy accretes its mass through
smooth infall of gas of primordial chemical composition (classical models) or
adopt mass accretion histories derived from the combination of merger trees
with semi-analytical modelling (cosmologically-motivated models). Furthermore,
we consider models with and without taking into account inhomogeneous mixing in
the ISM within the galaxy. The theoretical predictions are then compared to
each other and to the body of the available data. From this analysis, we
confirm previous findings that Bootes I has formed stars with very low
efficiency but, at variance with previous studies, we do not find a clear-cut
indication that supernova explosions have sustained long-lasting galactic-scale
outflows in this galaxy. Therefore, we suggest that external mechanisms such as
ram pressure stripping and tidal stripping are needed to explain the absence of
neutral gas in Bootes I today.Comment: 13 pages, 11 figures, accepted for publication in MNRA
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