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相关论文: ESO540-032: a Transition-Type Dwarf in the Sculpto…

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Spectroscopy and V,I CCD photometry of the dwarf irregular galaxy SBS 1129+576 are presented for the first time. The CCD images reveal a chain of compact H II regions within the elongated low-surface-brightness (LSB) component of the…

天体物理学 · 物理学 2009-11-07 N. G. Guseva , P. Papaderos , Y. I. Izotov , R. F. Green , K. J. Fricke , T. X. Thuan , K. J. Noeske

We present new near-IR and optical spectroscopic observations which confirm the redshift of the z=1.44 extremely red object ERO J164502+4626.4 (object 10 of Hu & Ridgway 1994) and a HST image which reveals a reflected-S-shaped morphology at…

天体物理学 · 物理学 2009-10-31 A. Dey , J. R. Graham , R. J. Ivison , I. Smail , G. S. Wright , M. C. Liu

Color-magnitude diagrams from deep, wide-field CCD photometry of the Sculptor dwarf spheroidal galaxy reveal that the red horizonal branch (RHB) stars are strongly concentrated towards the center of the galaxy relative to the dominant old…

天体物理学 · 物理学 2009-10-31 D. Hurley-Keller , M. Mateo , E. Grebel

We present $V$ and $I$ CCD photometry for $\sim360$ stars in the recently discovered dwarf galaxy Tucana. The large field investigated and the accurate photometric calibration make our data complementary to the deeper HST photometry. From…

天体物理学 · 物理学 2008-02-03 Ivo Saviane , Enrico V. Held , Giampaolo Piotto

We have obtained deep B and R-band CCD photometry for 5 dE galaxies that were previously identified on Schmidt films covering the Cen A group region. From a Fourier analysis of the R-band CCD images we determined the surface brightness…

天体物理学 · 物理学 2009-10-31 Helmut Jerjen , Ken C. Freeman , Bruno Binggeli

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…

天体物理学 · 物理学 2009-06-23 Leonardo Úbeda , J. Maíz-Apellániz , John MacKenty

Using deep two-band imaging from the Hubble Space Telescope, we measure the color-magnitude relations (CMR) of E/S0 galaxies in a set of 9 optically-selected clusters principally from the Red-Sequence Cluster Survey (RCS) at 0.9 < z < 1.23.…

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…

天体物理学 · 物理学 2015-06-24 Michael D. Gregg , Henry C. Ferguson , Dante Minniti , Nial Tanvir , Robin Catchpole

We present the metallicity distribution of a sample of 471 RR Lyrae (RRL) stars in the Sculptor dSph, obtained from the $I$-band Period-Luminosity relation. It is the first time that the early chemical evolution of a dwarf galaxy is…

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…

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

NGC 300 is a low-mass disk galaxy in the Sculptor group. In the literature, it has been identified as a pure exponential disk galaxy, as its luminosity profile could be well fitted with a single exponential law over many disk scale lengths…

HIZSS3 is an H I source in the Zone of Avoidance. Its radio characteristics are consistent with it being nearby (~ 1.8 Mpc) low-mass dwarf irregular (dIm) galaxy. It contains a modest H II region, but its stellar population has not been…

天体物理学 · 物理学 2009-11-10 David R. Silva , Philip Massey , Kathleen DeGioia-Eastwood , P. A. Henning

Previous evolutionary computations concerning stars with masses in the range of the ``Red Giants Transition Phase'' are extended to lower metallicities. Clusters isochrones for two values of the metallicity Z (Z=10E-4, 4E-4) and for ages…

天体物理学 · 物理学 2009-09-25 V. Castellani , S. Degl'Innocenti

We report the discovery of SDSSJ1049+5103, an overdensity of resolved blue stars at (\alpha_{2000}, \delta_{2000}) = (162.343, 51.051). This object appears to be an old, metal-poor stellar system at a distance of 45 +/- 10 kpc, with a…

We present new Very Large Array HI spectral line, archival Sloan Digital Sky Survey, and archival Spitzer Space Telescope imaging of eight star-forming blue compact dwarf galaxies that were selected to be optically compact (optical radii…

宇宙学与河外天体物理 · 物理学 2015-06-15 Hans P. Most , John M. Cannon , John J. Salzer , Jessica J. Rosenberg , Eric Engstrom , Palmer Fliss

(abridged) We present B,V,I CCD photometry of about 40000 stars in four regions of the Fornax dSph. Using the resultant CMDs, many already known age-tracers are investigated, and new CMD features are also detected: we show that blue HB…

天体物理学 · 物理学 2007-05-23 Ivo Saviane , Enrico V. Held , Gianpaolo Bertelli

We have obtained spectra of the yellow giant S1040 in the open cluster M67 using the Goddard High-Resolution Spectrograph (GHRS) and the Faint Object Spectrograph on the Hubble Space Telescope. S1040 is a single-lined spectroscopic binary…

天体物理学 · 物理学 2009-10-30 W. Landsman , J. Aparicio , P. Bergeron , R. Di Stefano , T. Stecher

We present a study of the evolved stellar populations in the dwarf spheroidal galaxy Fornax based on JHK imaging photometry. The observations cover an 18.5x18.5 arcmin central area with a mosaic of NTT/SOFI images. Our data sample all the…

天体物理学 · 物理学 2009-11-13 M. Gullieuszik , E. V. Held , L. Rizzi , I. Saviane , Y. Momany , S. Ortolani

To gain deeper insights into galaxy evolution and the mechanisms driving transitions between different galaxy morphologies, we analyse the connection between star formation rate and stellar mass for 231 galaxies spanning Hubble types E1-Sdm…

星系天体物理 · 物理学 2026-02-23 Veselina Kalinova , Keiichi Kodaira , Dario Colombo

We report the discovery of a compact object (R_e = 32 pc, M_B = -12.34 mag) at a projected distance of 9 kpc from Messier 59, a giant elliptical in the Virgo cluster. Using HST imaging and SDSS spectroscopy, both available in the Virtual…

天体物理学 · 物理学 2010-02-11 Igor V. Chilingarian , Gary A. Mamon