Stellar systems
Chemodynamics of compact stellar systems in NGC 5128: How similar are globular clusters ultra compact dwarfs and dwarfs galaxies?
... massive stellar systems are similar to those of both massive GCs contained within the Local Group and nuclear star clusters and ultra-compact dwarf galaxies ...massive stellar systems match ...
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On a New Parameter to Estimate the Helium Content in Old Stellar Systems
... ABSTRACT. We introduce a new parameter Δξ— the difference in magnitude between the red giant branch (RGB) bump and the point on the main sequence (MS) at the same color as the bump (which we call the “ benchmark ” ) — to ...
13
The HST/ACS Coma Cluster Survey V Compact stellar systems in the Coma Cluster
... In Fig. 9, we present the Faber & Jackson (1976) relation for a compilation of hot stellar systems. For elliptical galaxies, we take data from Faber et al. (1989), Geha, Guhathakurta & van der Marel ...
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Unveiling the architecture of the Fornax galaxy cluster with its different stellar systems
... Stellar systems complete in themselves was the basis of our definition of galaxies given by Edwin Hubble in 1926 , it was also the starting point for these nebulae to be recognized as extragalactic ...
171
Chemical composition of the stellar cluster Gaia1: No surprise behind Sirius
... The chemical composition of Gaia1 that we derived from MIKE spectra matches the composition of thin-disk stars and open clusters with similar metallicity well (see e.g. Pancino et al. 2010; Mishenina et al. 2015, and ...
6
The nature of UCDs: Internal dynamics from an expanded sample and homogeneous database
... the stellar population codes may not represent the globular cluster properties (see also Dabringhausen et ...pact stellar systems under investigation, and hence contributed to shaping the observed ...
17
Stellar substructures in the southern galactic hemisphere
... of stellar substructure located in the ...different stellar substructure in the southern Galactic halo ob- served by wide-field ...the stellar halo by a particular GC (NGC 7492), the Sgr satellite ...
164
Desarrollo de un sistema de informacin en la Sala de Apoyo a la Gestin Estratgica del Ministerio de Salud en Brasil
... implement systems and tools in an environment marked by diverse circumstances, systems and tools which are capable of unifying information into a single database for the purpose of decision- making and ...
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Null controllable sets and reachable sets for nonautonomous linear control systems
... x 0 = A(ω·t) x + B(ω·t) u(t) , ω ∈ Ω , (1.2) where Ω is a compact metric space, σ : R × Ω → Ω, (t, ω) 7→ ω·t is a continuous flow, and the matrix-valued functions A : Ω → M n×n ( R ) and B : Ω → M n×m ( R ) are ...
26
Massive Stellar X ray Sources in the Galactic Center
... wind at low ˙ M, which would make quiescent HMXBs in the Galactic center undetectable in X-rays (Liu & Li 2006). Single star scenarios also remain possible. O stars with strong magnetic fields can channel supersonic ...
5
GalaxiasEstrellas.doc
... En la década de lo cincuenta se descubrieron los quasar (quasi-stellar radio source), objetos este- lares mucho más pequeños que las galaxias (del orden de un millón de veces más pequeños que la Vía Láctea), que ...
7
Weighing the two stellar components of the Galactic bulge
... The second misconception is that the MP, spheroidal compo- nent represents a minor contribution to the total stellar mass of the bulge. This idea is based on the fact that in Baade’s Window, by far the most ...
6
Discovery of a thin stellar stream in the SLAMS survey
... Thin stellar streams in the Galactic halo may provide the first evidence for such a population, the basic idea being that a subhalo interaction can induce an observable density perturbation – a gap – in the ...
10
Discovery of four gravitationally lensed quasars from the Sloan Digital Sky Survey
... two stellar components is ...two stellar components have broad emission lines (C iii] and Mg ii) at the same wavelengths, supporting the lensing hypothesis of this ...
7
Top heavy integrated galactic stellar initial mass functions in starbursts
... in Fig. 4 the IGIMF results are in good agreement with the con- straints for the Galactic and M31 bulge (filled circle with error bar; Ballero et al. 2007a), as well as the Wilkins et al. (2008) constrains for the ...
8
Overview of semi sinusoidal stellar variability with the CoRoT satellite
... Figure 9 shows the color–magnitude diagram by compar- ing the CoRoT parent sample of 124 471 LCs (in black) with our final sample of 4206 stars (in red). This comparison in- dicates that some more biases were introduced ...
12
MEIA SYSTEMS: Membrane Encrypted Information Applications Systems
... P-systems evolve, which makes it change upon time; therefore it is a dynamic system. Every time that there is a change on the p-system we will say that the P-system is in a new transition. The step from one ...
7
Stellar population properties for a sample of hard X ray AGNs
... The values of the mass-weighted age and metallicity that we obtained when considering only one stellar population (i.e. the one dominating the mass) are shown in Fig. 6 on the left and right panel, respectively. ...
9
Implementation of algorithms for radar real-time signals processing using a microprocessor based platform
... Not in all embedded system application is needed to include an operating system, even less common to include a real time operating system, the decision has to do with the complexity of the application, the need of finish ...
52
Stellar evolution and variability in the pre ZAHB phase
... Bearing these di ffi culties in mind, Catelan (2005, 2007) sug- gested an alternative approach for the detection of pre-ZAHB stars, namely, through stellar pulsations. Indeed, some pre- ZAHB stars are expected to ...
8