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In this contribution initial results from colour-magnitude diagrams for five dEs in the M81 group are presented. The colour-magnitude diagrams, derived from HST/ACS images, reach well below the red giant branch tip and allow evaluation of…

Astrophysics · Physics 2007-05-23 G. S. Da Costa

We study the red giant populations of two dE galaxies, AM 1339-445 and AM 1343-452, with the aim of investigating the number and luminosity of any upper asymptotic giant branch (AGB) stars present. The galaxies are members of the Centaurus…

Astrophysics · Physics 2009-11-11 M. Rejkuba , G. S. Da Costa , H. Jerjen , M. Zoccali , B. Binggeli

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)…

We present a study aimed at deriving constraints on star formation at intermediate ages from the evolved stellar populations in the dwarf irregular galaxy UKS2323-326. These observations were also intended to demonstrate the scientific…

Deep g'r'i'z' images obtained with the Gemini Multi-Object Spectrograph are used to investigate the stellar content in the outer regions of the nearby Sc galaxies NGC 2403 and M33. The red giant branch tip occurs at i' = 23.6 +/- 0.1 in NGC…

Astrophysics · Physics 2009-11-07 T. J. Davidge

Near-infrared images obtained with the CFHT AOB are used to investigate the stellar content of the Local Group elliptical galaxy M32. Observations of a field 2.3 arcmin from the galaxy center reveal a large population of AGB stars, and…

Astrophysics · Physics 2009-10-31 T. J. Davidge

We investigate the utility of the asymptotic giant branch (AGB) and the red giant branch (RGB) as probes of the star formation history (SFH) of the nearby (D=2.5 Mpc) dwarf irregular galaxy, KKH 98. Near-infrared (IR) Keck Laser Guide Star…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-18 J. Melbourne , B. Williams , J. Dalcanton , S. M. Ammons , C. Max , D. C. Koo , Leo Girardi , A. Dolphin

We have tested the reliability of the red giant branch (RGB) as a metallicity indicator accounting for observational errors as well as the complexity of star formation histories (SFHs) and chemical evolution histories observed in various…

Solar and Stellar Astrophysics · Physics 2015-06-03 Antonio J. Ordoñez , Ata Sarajedini

We explore the effects of stellar population models on estimating star formation histories, ages and masses of high redshift galaxies. The focus is on the Thermally-Pulsing Asymptotic Giant Branch (TP-AGB) phase of stellar evolution, whose…

Astrophysics · Physics 2008-11-26 C. Maraston , E. Daddi , A. Renzini , A. Cimatti , M. Dickinson , C. Papovich , A. Pasquali , N. Pirzkal

Using the Near Infrared Camera and Multi-Object Spectrometer (NICMOS) on board the Hubble Space Telescope, we have obtained F110W (J-band) and F160W (H-band) images of three fields in NGC3379, a nearby normal giant elliptical galaxy. These…

Astrophysics · Physics 2015-06-24 Michael D. Gregg , Henry C. Ferguson , Dante Minniti , Nial Tanvir , Robin Catchpole

Asymptotic giant branch stars are essential contributors to the near and mid-IR emission of intermediate age (0.1-1Gyr old) stellar populations. Detecting this light sets constraints on the star formation history in galaxies and,…

Astrophysics · Physics 2007-05-23 A. Lancon

We present color-magnitude diagrams and luminosity functions of stars in two halo regions of the irregular galaxy in M82, based on F555W and F814W photometry taken with the Hubble Space Telescope and Wide Field Planetary Camera 2. The…

Astrophysics · Physics 2009-10-31 Shoko Sakai , Barry Madore

We present UBVRI surface photometry for 16 dwarf elliptical galaxies in the Virgo Cluster with previously measured kinematic properties. The global optical colors are red, with median values for the sample of 0.24 +/- 0.03 in (U-B), 0.77…

Astrophysics · Physics 2009-11-10 L. van Zee , E. J. Barton , E. D. Skillman

With the William Herschel Telescope in La Palma we made IJKs observations of an area of about 40'x30' of the Local Group galaxy Draco. This allows us to describe Draco's late-type stellar population across the whole galaxy at a photometric…

Astrophysics · Physics 2009-11-11 M. -R. L. Cioni , H. J. Habing

We present new stellar population models that include the contribution of the Thermally Pulsing Asymptotic Giant Branch (TP-AGB) phase also in the synthetic spectral energy distribution (SED). The TP-AGB phase is essential for a correct…

Astrophysics · Physics 2009-11-10 Claudia Maraston

We investigate the resolved stellar content of early-type dwarf galaxies in the CenA group, in order to estimate the fraction of their intermediate-age populations. We use near-infrared photometric data taken with the VLT/ISAAC instrument,…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-27 D. Crnojević , M. Rejkuba , E. K. Grebel , G. Da Costa , H. Jerjen

This is the first of a series of papers devoted to a global study of the photometric properties of the red stellar sequences in a complete sample of the Large Magellanic Cloud clusters, by means of near infrared array photometry. Deep…

Astrophysics · Physics 2009-11-10 Francesco R. Ferraro , Livia Origlia , Vincenzo Testa , Claudia Maraston

(Abridged) We have investigated the reliability of the widely used I-band Tip of the RGB relative distances for a sample of Local Group galaxies with complex Star Formation Histories (SFR) and Age Metallicity Relationships (AMR) namely the…

Astrophysics · Physics 2009-11-10 Maurizio Salaris , Leo Girardi

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…

Astrophysics · Physics 2008-11-26 A. Mucciarelli , L. Origlia , F. R. Ferraro , C. Maraston , V. Testa

Major progress has been achieved in recent years in mapping the properties of passively-evolving, early-type galaxies (ETG) from the local universe all the way to redshift ~2. Here, age and metallicity estimates for local cluster and field…

Astrophysics · Physics 2011-02-11 Alvio Renzini
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