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

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We have obtained V and I-band photometry for about 700 stars in the field of the dwarf irregular galaxy IC 5152, previously considered a possible member of the Local Group. Deep VI color-magnitude diagrams are presented of the main body of…

天体物理学 · 物理学 2009-10-31 Albert A. Zijlstra , Dante Minniti

We present the Two Micron All Sky Survey (2MASS) (J-K, K) color-magnitude diagram for the region within 1 degree of the center of the Sagittarius dwarf spheroidal galaxy. Using the slope of the red giant branch (RGB), we determine a mean…

天体物理学 · 物理学 2009-11-07 A. A. Cole

Low resolution (4.5 to 5 Angstroem) spectra of 58 blue supergiant stars distributed over the disk of the Magellanic spiral galaxy NGC 55 in the Sculptor group are analyzed by means of non-LTE techniques to determine stellar temperatures,…

Deep J, H, and K images are used to probe the evolved stellar contents in the central regions of the Sculptor group galaxies NGC55, NGC300, and NGC7793. The brightest stars are massive red supergiants (RSGs) with K ~ 15 - 15.5. The peak RSG…

天体物理学 · 物理学 2009-10-30 T. J. Davidge

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,…

宇宙学与河外天体物理 · 物理学 2015-05-27 D. Crnojević , M. Rejkuba , E. K. Grebel , G. Da Costa , H. Jerjen

We present an analysis of Hubble Space Telescope/WFPC2 images of nine nearby galaxies in Sculptor. We derive their distances from the luminosity of the tip of the red giant branch stars with a typical accuracy of ~ 12%. Their distances are…

We use two-band imaging data from the Advanced Camera for Surveys on board the Hubble Space Telescope for a detailed study of NGC1533, an SB0 galaxy in the Dorado group surrounded by a ring of HI. NGC1533 appears to be completing a…

天体物理学 · 物理学 2007-10-05 Regina Barber DeGraaff , John P. Blakeslee , Gerhardt R. Meurer , Mary E. Putman

The star EPIC 210894022 has been identified from a light curve acquired through the K2 space mission as possibly orbited by a transiting planet. Our aim is to confirm the planetary nature of the object and derive its fundamental parameters.…

"Fossil" galaxy groups, each dominated by a relatively isolated giant elliptical galaxy, have many properties intermediate between groups and clusters of galaxies. We used the {\sl Suzaku} X-ray observatory to observe the X-ray brightest…

宇宙学与河外天体物理 · 物理学 2015-06-16 Yuanyuan Su , Raymond E. White , Eric D. Miller

We present HST WFPC2 V and I images and GHRS UV spectrophotometry of the spectral regions around Ly$_alpha$ and OI 1302 of the extremely metal-deficient (Z~Zsun/41) blue compact dwarf (BCD) galaxy SBS 0335-052. All the star formation in the…

天体物理学 · 物理学 2009-10-28 Trinh X. Thuan , Yu. I. Izotov , V. A. Lipovetsky

We present optical VLT spectroscopy of 16 dwarf elliptical galaxies (or dEs) comparable in mass to NGC 205, and belonging to the Fornax cluster and to nearby groups of galaxies. Using ULySS and STECKMAP, we derive radial profiles of the…

宇宙学与河外天体物理 · 物理学 2015-05-13 Mina Koleva , Sven De Rijcke , Philippe Prugniel , Werner W. Zeilinger , Dolf Michielsen

We have performed the first detailed simulation of the horizontal branch of the Sculptor dwarf spheroidal galaxy by means of synthetic modelling techniques,taking consistently into account the star formation history and metallicity…

星系天体物理 · 物理学 2015-06-17 Maurizio Salaris , Thomas de Boer , Eline Tolstoy , Giuliana Fiorentino , Santi Cassisi

We aim at constraining evolutionary models at low mass and young ages by identifying interesting transiting system members of the nearest OB association to the Sun, Upper Scorpius, targeted by the Kepler mission. We produced light curves…

We present the first (V,V-I) Color -- Magnitude Diagram (CMD) for the poorly studied globular cluster NGC 5634. The CMD shows a steep Red Giant Branch (RGB) and a predominantly blue Horizontal Branch (HB): both these characteristics suggest…

天体物理学 · 物理学 2009-11-07 Michele Bellazzini , Francesco R. Ferraro , Rodrigo Ibata

NGC 4382 is a merger-remnant galaxy that has been classified as morphological type E2, S0, and even Sa. In this work, we performed a photometric and spectroscopic analysis of the globular cluster (GC) system of this peculiar galaxy in order…

The Advanced Camera for Surveys (ACS) on HST has been used to image two fields in the core of the Virgo cluster that contain a number of dwarf elliptical galaxies. The combined F555W and F814W images have resolved red giant stars in these…

天体物理学 · 物理学 2008-11-26 Nelson Caldwell

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…

天体物理学 · 物理学 2009-11-10 S. A. Pustilnik , A. G. Pramskij , A. Y. Kniazev

We have observed three fields of the Coma cluster of galaxies with a narrow band (modified Stromgren) filter system. Observed galaxies include 31 in the vicinity of NGC 4889, 48 near NGC 4874, and 60 near NGC 4839 complete to M_5500=-18 in…

天体物理学 · 物理学 2009-11-07 A. Odell , J. Schombert , K. Rakos

We present a new discrete chemo-dynamical axisymmetric modeling technique, which we apply to the dwarf spheroidal galaxy Sculptor. The major improvement over previous Jeans models is that realistic chemical distributions are included…

星系天体物理 · 物理学 2016-09-07 Ling Zhu , Glenn van de Ven , Laura L. Watkins , Lorenzo Posti

We report the discovery of a rare isolated group of five dwarf galaxies located at z = 0.0086 ($D$ = 36 Mpc). All member galaxies are star-forming, blue, and gas-rich with $g-r$ indices ranging from 0.2 to 0.6 mag, and two of them show…

星系天体物理 · 物理学 2024-11-18 Sanjaya Paudel , Cristiano G. Sabiu , Suk-Jin Yoon , Pierre-Alain Duc , Jaewon Yoo , Oliver Müller