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相关论文: The Carina Project: II. Stellar Populations

200 篇论文

We present a detailed analysis of the Horizontal Branch of the Carina Dwarf Spheroidal Galaxy by means of synthetic modelling techniques, taking consistently into account the star formation history and metallicity evolution as determined…

星系天体物理 · 物理学 2015-11-04 Alessandro Savino , Maurizio Salaris , Eline Tolstoy

We have analyzed deep B and V photometry of the Carina dwarf spheroidal reaching below the old main-sequence turnoff to about V = 25. Using simulated color-magnitude diagrams to model a range of star formation scenarios, we have extracted a…

天体物理学 · 物理学 2009-10-30 Denise Hurley-Keller , Mario Mateo , James Nemec

We study the stellar populations, star formation histories and star formation properties for a sample of blue compact dwarf galaxies (BCDs) selected by cross-correlating the Gil de Paz et al. (2003) sample with the Sloan Digital Sky Survey…

宇宙学与河外天体物理 · 物理学 2015-03-17 Yinghe Zhao , Qiusheng Gu , Yu Gao

We analyse the stellar content of a large number of HII galaxies from the continua and absorption features of their spectra using population synthesis methods, in order to gain information about the star formation histories of these…

天体物理学 · 物理学 2009-11-10 P. Westera , F. Cuisinier , E. Telles , C. Kehrig

We report on the detection of Main Sequence stars belonging to the recently identified Canis Major galaxy in a field located at ~ 4.2 deg from the center of the stellar system. With Main Sequence fitting we obtain a distance modulus…

天体物理学 · 物理学 2009-11-10 M. Bellazzini , R. Ibata , L. Monaco , N. Martin , M. J. Irwin , G. F. Lewis

We use the first release of the SDSS/MaStar stellar library comprising ~9000, high S/N spectra, to calculate integrated spectra of stellar population models. The models extend over the wavelength range 0.36-1.03 micron and share the same…

We present deep CCD photometry of a field in the newly discovered dwarf spheroidal galaxy in Sagittarius (hereafter Sgr), and of a nearby control field. These data (totaling ~3.5 hrs exposure time in V and I) were used to produce…

天体物理学 · 物理学 2009-10-22 Mario Mateo , A. Udalski , M. Szymanski , J. Kaluzny , M. Kubiak , W. Krzeminski

We report the detection of 388 pulsating variable stars (and some additional miscellaneous variables) in the Carina dSph galaxy over an area covering the full visible extent of the galaxy and extending a few times beyond its photometric…

太阳与恒星天体物理 · 物理学 2015-06-17 A. Katherina Vivas , Mario Mateo

We have obtained V and I-band photometry for about 17500 stars in the field of the dwarf irregular galaxy NGC3109, located in the outskirts of the Local Group. The photometry allows us to study the stellar populations present inside and…

天体物理学 · 物理学 2009-10-31 Dante Minniti , Albert Zijlstra , M. Victoria Alonso

Recent results on the detection of substructure in dwarf spheroidal galaxies are discussed. In most cases they show that, when a galaxy experiences multiple SF episodes, the intermediate age population is more centrally concentrated than…

天体物理学 · 物理学 2007-05-23 Ivo Saviane , Enrico V. Held , Yazan Momany , Luca Rizzi

We present new optical (BVI) time-series data for the evolved variable stars in the Carina dwarf spheroidal galaxy. The quality of the data and the observing strategy allowed us to identify 14 new variable stars. Eight out of the 14 are RR…

We have traced the spatial distributions of intermediate-age and old stars in nine dwarf galaxies in the distant parts of the Local Group, using multi-epoch 3.6 and 4.5 micron data from the DUST in Nearby Galaxies with Spitzer (DUSTiNGS)…

In this paper, we show that the optically bright stars above the tip of the first red giant branch (TRGB) in the color magnitude (CM) diagrams of nearby dwarf elliptical (dE) galaxies, commonly interpreted as indication of the existence of…

天体物理学 · 物理学 2009-10-30 D. Martinez-Delgado , A. Aparicio

We analyze in detail the spatial distribution and kinematic properties of two different stellar populations in Andromeda II (And II) dwarf spheroidal galaxy. We obtained their detailed surface density maps, together with their radial…

星系天体物理 · 物理学 2017-06-28 Andrés del Pino , Ewa L. Lokas , Sebastian L. Hidalgo , Sylvain Fouquet

We present the first deep color-magnitude diagram of the Canes Venatici I (CVnI) dwarf galaxy from observations with the wide field Large Binocular Camera on the Large Binocular Telescope. Reaching down to the main-sequence turnoff of the…

(Abridged) We present deep, sub-horizontal branch, multi-colour photometry of the Andromeda II dwarf spheroidal (And II dSph) taken with Subaru Suprime-Cam. We identify a red clump population in this galaxy, the first time this feature has…

天体物理学 · 物理学 2009-06-23 Alan McConnachie , Nobuo Arimoto , Mike Irwin

We use Subaru Suprime-Cam and VLT FORS1 photometry of the dwarf galaxy DDO210 to study the global stellar content and structural properties of a transition-type galaxy (with properties intermediate between dwarf irregular and dwarf…

天体物理学 · 物理学 2009-11-11 Alan W. McConnachie , Nobuo Arimoto , Mike Irwin , Eline Tolstoy

We present new deep $VI$ ground-based photometry of the Local Group dwarf galaxy Phoenix. Our results confirm that this galaxy is mainly dominated by red stars, with some blue plume stars indicating recent (100 Myr old) star formation in…

天体物理学 · 物理学 2009-10-31 D. Martinez-Delgado , C. Gallart , A. Aparicio

We present a statistically decontaminated Color Magnitude Diagram of a 1 deg X 1 deg field in the core of the Sagittarius dSph galaxy. Coupling this CMD with the most recent metallicity distributions obtained from high resolution…

天体物理学 · 物理学 2009-11-11 M. Bellazzini , M. Correnti , F. R. Ferraro , L. Monaco , P. Montegriffo

We present metallicities for 487 red giants in the Carina dwarf spheroidal (dSph) galaxy that were obtained from FLAMES low-resolution Ca triplet (CaT) spectroscopy. We find a mean [Fe/H] of -1.91 dex with an intrinsic dispersion of 0.25…

天体物理学 · 物理学 2007-05-23 A. Koch , E. K. Grebel , D. Harbeck , M. I. Wilkinson , J. T. Kleyna , G. F. Gilmore , R. F. G. Wyse , N. W. Evans