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We have obtained 1-2 A resolution optical Echellette spectra of the nuclear star cluster in the nearby starburst galaxy NGC 4449. The light is clearly dominated by a very young (6-10 Myr) population of stars. For our age dating, we have…

Astrophysics · Physics 2009-10-31 T. Boeker , R. P. van der Marel , L. Mazzuca , H. -W. Rix , G. Rudnick , L. C. Ho , J. C. Shields

Newly obtained HST/WFPC2 images of the disturbed elliptical galaxy NGC 5018 show that the average amount of internal reddening due to the its complex ``dust web'' is as low as E(B-V)~0.02 within the IUE aperture, thus implying that its…

Astrophysics · Physics 2007-05-23 Lucio M. Buson , Francesco Bertola , David Burstein , Michele Cappellari

The distribution of galaxy properties in groups and clusters holds important information on galaxy evolution and growth of structure in the Universe. While clusters have received appreciable attention in this regard, the role of groups as…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-13 J. Trevor Mendel , Robert N. Proctor , Jesper Rasmussen , Sarah Brough , Duncan A. Forbes

We present the results of a detailed UV-optical study of the nearby dwarf starburst galaxy NGC 4214 using multifilter HST/WFPC2+STIS photometry. The stellar extinction is found to be quite patchy, with some areas having values of…

Astrophysics · Physics 2009-06-23 Leonardo Úbeda , J. Maíz-Apellániz , John MacKenty

We present the analysis of Lick absorption-line indices from three separate long-slit spectroscopic observations of the nearby isolated elliptical galaxy NGC 821. The three data sets present a consistent picture of the stellar population…

Astrophysics · Physics 2016-08-30 Robert N. Proctor , Duncan A. Forbes , Amy Forestell , Karl Gebhardt

This paper presents a quantitative analysis of the stellar content in the Local Group dwarf irregular galaxy NGC 6822 by comparing stellar evolution models and observations in color-magnitude diagrams (CMDs) and color-color diagrams…

Drawing from the LEGA-C dataset, we present the spectroscopic view of the stellar population across a large volume- and mass-selected sample of galaxies at large lookback time. We measure the 4000\AA\ break (D$_n$4000) and Balmer absorption…

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…

Astrophysics · Physics 2009-11-10 P. Westera , F. Cuisinier , E. Telles , C. Kehrig

We present colour-magnitude diagrams for two rich (~10^4 Msun) Large Magellanic Cloud star clusters with ages ~10^7 years, constructed from optical and near-infrared data obtained with the Hubble Space Telescope. These data are part of an…

We have obtained Keck spectra for 16 globular clusters (GCs) associated with the merger remnant elliptical NGC 1052, as well as a long-slit spectrum of the galaxy. We derive ages, metallicities and abundance ratios from simple stellar…

We map optical and near-infrared (NIR) stellar population properties of the inner 320$\times$535pc$^2$ of the elliptical galaxy NGC1052. The optical and NIR spectra were obtained using the Gemini Integral Field Units of the GMOS instrument…

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…

Astrophysics · Physics 2009-10-31 Dante Minniti , Albert Zijlstra , M. Victoria Alonso

We present deep optical and near-infrared imaging of the rich cluster A2218 at z=0.17. Our optical imaging comes from new multicolour Hubble Space Telescope WFPC2 observations in the F450W (B), F606W (V) and F814W (I) passbands. These…

Astrophysics · Physics 2015-06-24 Ian Smail , Harald Kuntschner , T. Kodama , G. P. Smith , C. Packham , A. S. Fruchter , R. N. Hook

We have extracted PSF-fitted stellar photometry from near-ultraviolet, optical and near-infrared images, obtained with the Hubble Space Telescope, of the nearby (D ~ 5.5 Mpc) SBm galaxy NGC 1311. The ultraviolet and optical data reveal a…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-19 Paul B. Eskridge , Rogier A. Windhorst , Violet A. Mager , Rolf A. Jansen

(Abridged for arXiv) The history of the mass assembly of brightest cluster galaxies may be studied by the mapping the stellar populations at large radial distances from the galaxy centre. We provide extended and robust measurements of the…

We present the results of an infrared photometric survey performed with NICS@TNG in the nearby starburst galaxy NGC 4214. We derived accurate integrated JK magnitudes of 10 young massive clusters and compared them with the already available…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-15 A. Sollima , R. G. Gratton , E. Carretta , A. Bragaglia , S. Lucatello

The radial distributions of the Mg2 and Fe5270 Lick spectral indices have been measured to large radial distances on the disks of NGC 4303 and NGC 4535 using an imaging technique based on interference filters. These data, added to those of…

Astrophysics · Physics 2009-10-31 M. Molla , E. Hardy , D. Beauchamp

We present new integrated light spectroscopy of globular clusters (GCs) in NGC 5128 in order to measure radial velocities and derive ages, metallicities, and alpha-element abundance ratios. Using Gemini-S 8-m/GMOS, we obtained spectroscopy…

Astrophysics of Galaxies · Physics 2014-11-20 Kristin A. Woodley , William E. Harris , Thomas H. Puzia , Matias Gomez , Gretchen L. H. Harris , Doug Geisler

We study the central (inner few hundred parsecs) stellar populations of four starburst galaxies (NGC34, NGC1614, NGC3310 and NGC7714) in the near-infrared (NIR), from 0.8 to 2.4microns, by fitting combinations of stellar population models…

Astrophysics · Physics 2009-11-13 R. Riffel , M. G. Pastoriza , A. Rodriguez-Ardila , C. Maraston

We present [Fe/H], ages, and Ca abundances for an initial sample of 10 globular clusters in NGC 5128 obtained from high resolution, high signal-to-noise ratio echelle spectra of their integrated light. All abundances and ages are obtained…

Astrophysics of Galaxies · Physics 2015-06-16 J. E. Colucci , M. F. Duran , R. A. Bernstein , A. McWilliam
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