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Related papers: Anomalous Stellar Populations in LSB Galaxies

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We present UBVI surface photometry of a sample of low surface brightness (LSB) disk galaxies. LSB disk galaxies are fairly well described as exponential disks with no preferred value for either scale length, central surface brightness, or…

Astrophysics · Physics 2009-10-22 Stacy McGaugh , Greg Bothun

We investigate the stellar masses of the class of star-forming objects known as Luminous Compact Blue Galaxies (LCBGs) by studying a sample of galaxies in the distant cluster MS$~$0451.6-0305 at $z\approx0.54$ with ground-based multicolor…

Astrophysics of Galaxies · Physics 2017-08-02 S. M. Randriamampandry , S. M. Crawford , M. A. Bershady , G. D. Wirth , C. M. Cress

We study the Galactic distribution of ~10,000 Asymptotic Giant Branch (AGB) stars selected by IRAS colors and variability index. The distance to each star is estimated by assuming a narrow luminosity function and a model-derived bolometric…

Astrophysics · Physics 2009-11-07 T. Jackson , Z. Ivezic , G. R. Knapp

Giant Low Surface Brightness Galaxies (GLSBGs) are fundamentally distinct from normal galaxies (LSBGs) in star formation and evolution. In this work, we collected 27 local GLSBGs. They have high stellar masses (M*>10^10 Msolar) and low…

Astrophysics of Galaxies · Physics 2023-11-14 Wei Du , Cheng Cheng , Pengliang Du , Lin Du , Hong Wu

We have discovered two new high redshift (z=2.38) galaxies, near the previously known z=2.38 galaxy 2139-4434 B1 (Francis et al. 1996). All three galaxies are strong Ly-alpha emitters, and have much redder continuum colors (I-K about 5)…

Astrophysics · Physics 2009-10-30 Paul J. Francis , Bruce E. Woodgate , Anthony C. Danks

We present V and I photometry of the resolved stars in the cometary dwarf irregular galaxy NGC 2366, using Wide Field Planetary Camera 2 images obtained with the Hubble Space Telescope. The resulting color-magnitude diagram reaches down to…

Astrophysics · Physics 2009-11-10 T. X. Thuan , Y. I. Izotov

We trace the full evolution of low- and intermediate-mass stars ($1 M_{\odot} \leq M \leq 8M_{\odot}$) during the Asymptotic Giant Branch (AGB) phase in the {\it Spitzer} two-color and color-magnitude diagrams. We follow the formation and…

Solar and Stellar Astrophysics · Physics 2015-06-19 F. Dell'Agli , P. Ventura , D. A. García Hernández , R. Schneider , M. Di Criscienzo , E. Brocato , F. D'Antona , C. Rossi

We use deep Hubble Space Telescope imaging in the outskirts of the nearby spiral M101 to study stellar populations in the galaxy's outer disk and halo. Our ACS field lies 17.6 arcmin (36 kpc) from the center of M101 and targets the blue "NE…

Astrophysics of Galaxies · Physics 2018-08-08 J. Christopher Mihos , Patrick R Durrell , John J Feldmeier , Paul Harding , Aaron E Watkins

We have carried out a search for optically visible post-Asymptotic Giant Branch (post-AGB) stars in the Large Magellanic Cloud (LMC). First, we selected candidates with a mid-IR excess and then obtained their optical spectra. We…

Solar and Stellar Astrophysics · Physics 2015-10-19 Devika Kamath , Peter R. Wood , Hans Van Winckel

We serendipitously find a new nearby Low Surface Brightness (LSB) galaxy from SDSS database. We estimate oxygen abundance of its H II region SDSS J121811.0+465501.2 from electron temperature, as well as for another H II region, SDSS…

Astrophysics · Physics 2008-11-26 Y. C. Liang , J. Y. Hu , F. S. Liu , Z. T. Liu

Asymptotic giant branch (AGB) stars in the globular cluster NGC6752 have been found to exhibit some chemical peculiarities with respect to the red giant branch (RGB) stars. A discrepancy between [FeI/H] and [FeII/H] (not observed in RGB…

Solar and Stellar Astrophysics · Physics 2019-01-23 A. Mucciarelli , E. Lapenna , C. Lardo , P. Bonifacio , F. R. Ferraro , B. Lanzoni

We have collected UVES-FLAMES high-resolution spectra for a sample of 6 asymptotic giant branch (AGB) and 13 red giant branch (RGB) stars in the Galactic globular cluster M62 (NGC6266). Here we present the detailed abundance analysis of…

Solar and Stellar Astrophysics · Physics 2015-11-11 E. Lapenna , A. Mucciarelli , F. R. Ferraro , L. Origlia , B. Lanzoni , D. Massari , E. Dalessandro

[Abridged] In recent years the view of Galactic globular clusters as simple stellar populations has changed dramatically, as it is now thought that basically all GCs host multiple stellar populations, each with its own chemical abundance…

Solar and Stellar Astrophysics · Physics 2014-11-19 Santi Cassisi , Maurizio Salaris , Adriano Pietrinferni , Jorick S. Vink , Matteo Monelli

We recently reported the discovery of prominent features from the thermally pulsing asymptotic giant branch (TP-AGB) phase in the near-IR rest-frame of a massive quiescent galaxy (QG) at z~1 observed with JWST, which set strong constraints…

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

In this proceeding we present the results from a study of very high-redshift galaxies with the newly commissioned Wide Field Camera 3 on the Hubble Space Telescope. With the deepest near-infrared data ever taken, we discovered 31 galaxies…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-19 Steven L. Finkelstein

We present the results of deep multicolour CCD imaging with the 6-m telescope of the pair of extremely metal-deficient gas-rich dwarf galaxies SBS 0335-052 E and W. The total magnitudes in U,B,V,R,I bands and the integrated fluxes of…

Astrophysics · Physics 2009-11-10 S. A. Pustilnik , A. G. Pramskij , A. Y. Kniazev

We analyze the spectral energy distributions (SEDs) of Lyman break galaxies (LBGs) at z=1-3 selected using the Hubble Space Telescope (HST) Wide Field Camera 3 (WFC3) UVIS channel filters. These HST/WFC3 observations cover about 50 sq.…

We present resolved-star VI photometry of the Local Group dwarf irregular galaxy IC1613 reaching I~23.5, obtained with the wide-field camera at the 2.5m Isaac Newton Telescope. A fit to the stellar density distribution shows an exponential…

We present UV images of M 31 and M 32, as observed by HST with the refurbished FOC. The galaxies were observed through the F175W and F275W filters, allowing the construction of color magnitude diagrams (CMDs) for the hundreds of detected…

Astrophysics · Physics 2009-10-30 T. M. Brown , H. C. Ferguson , S. A. Stanford , J. -M. Deharveng , A. F. Davidsen