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相关论文: Ultra-Compact Dwarf Candidates Near the Lensing Ga…

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We present preliminary results of the search for Ultra-compact dwarf galaxies in the central region of the Antlia cluster. This new kind of stellar system has brightness, mass and size between those observed in globular clusters and…

宇宙学与河外天体物理 · 物理学 2009-12-11 J. P. Caso , L. P. Bassino , A. V. Smith Castelli

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

The M31 satellite galaxy M32 has long been considered an object of unique properties, being the most extreme example of the very rare compact elliptical galaxy class. Here we present the spectroscopic discovery of two M32 twins in the…

天体物理学 · 物理学 2009-11-10 S. Mieske , L. Infante , M. Hilker , G. Hertling , J. P. Blakeslee , N. Benitez , H. Ford , K. Zekser

We report on the discovery of three bright, strongly-lensed objects behind Abell 1703 and CL0024+16 from a dropout search over 25 square arcminutes of deep NICMOS data, with deep ACS optical coverage. They are undetected in the deep ACS…

宇宙学与河外天体物理 · 物理学 2010-01-15 W. Zheng , L. D. Bradley , R. J. Bouwens , H. C. Ford , G. D. Illingworth , N. Benitez , T. Broadhurst , B. Frye , L. Infante , M. J. Jee , V. Motta , X. W. Shu , A. Zitrin

The origin of ultra-compact dwarfs (UCDs)--objects larger and more massive than typical globular clusters (GCs), but more compact than typical dwarf galaxies--has been hotly debated in the 15 years since their discovery. Even whether UCDs…

We review some properties of ultracompact dwarf galaxies (UCDs) in Fornax and of their brighter counterparts in Abell 1689, among which are two M32 twins, and discuss various possible UCD formation scenarios. We note that it is…

天体物理学 · 物理学 2009-11-11 S. Mieske , M. Hilker , L. Infante

In this work, we extend the catalog of low-surface brightness (LSB) galaxies, including Ultra-Diffuse Galaxy (UDG) candidates, within $\approx 0.4R_{vir}$ of the Hydra I cluster of galaxies, based on deep images from the VST Early-type…

The local universe is still full of hidden dwarf galaxies to be discovered using deep imaging campaigns. Here we present the third paper in a series to search for low-surface brightness dwarf galaxies around nearby isolated luminous host…

星系天体物理 · 物理学 2025-04-17 Oliver Müller , Helmut Jerjen , Salvatore Taibi , Nick Heesters , Ethan Crosby , Marcel S. Pawlowski

We study the population of ultra-diffuse galaxies (UDGs) in a set of eight nearby ($z <$ 0.035) galaxy clusters, from the Kapteyn IAC WEAVE INT Clusters Survey ($\texttt{KIWICS}$). We report the discovery of 442 UDG candidates in our eight…

(abridged) We present the first results of our deep survey of lensing clusters aimed at constraining the abundance of star-forming galaxies at z~6-10. Deep near-IR photometry of two lensing clusters (A1835 and AC114) was obtained with…

天体物理学 · 物理学 2009-11-11 Johan Richard , Roser Pello , Daniel Schaerer , Jean-Francois Le Borgne , Jean-Paul Kneib

In this contribution the discovery and properties of ultra-compact dwarf galaxies are presented, and their possible origin is discussed. This new type of galaxy resides in the cores of galaxy clusters. In the fundamental plane diagram of…

天体物理学 · 物理学 2007-05-23 Michael Hilker , Steffen Mieske

We present a study of the population of bright early-type dwarf galaxies in the multiple-cluster system Abell 901/902. We use data from the STAGES survey and COMBO-17 to investigate the relation between the color and structural properties…

Systematic studies have revealed hundreds of ultra-compact dwarf galaxies (UCDs) in the nearby Universe. With half-light radii $r_h$ of approximately 10-100 parsecs and stellar masses $M_*$ $\approx$ $10^6-10^8$ solar masses, UCDs are among…

We present the detection of a large population of ultra diffuse galaxies (UDGs) in two massive galaxy clusters, Abell S1063 at $z=0.348$ and Abell 2744 at $z=0.308$, based on F814W and F105W images in the Hubble Frontier Fields Program. We…

星系天体物理 · 物理学 2017-08-09 Myung Gyoon Lee , Jisu Kang , Jeong Hwan Lee , In Sung Jang

We present a homogeneous catalog of 275 large (effective radius $\gtrsim$ 5.3 arcsec) ultra-diffuse galaxy (UDG) candidates lying within an $\approx$ 290 square degree region surrounding the Coma cluster. The catalog results from our…

We present an Ultra-Cool Dwarf (UCD) catalogue compiled from low southern Galactic latitudes and mid-plane, from a cross-correlation of the 2MASS and SuperCOSMOS surveys. The catalogue contains 246 members identified from 5042 sq. deg.…

太阳与恒星天体物理 · 物理学 2015-06-04 S. L. Folkes , D. J. Pinfield , H. R. A. Jones , R. Kurtev , Z. Zhang , M. C. Gálvez-Ortiz , F. Marocco , A. C. Day-Jones , J. R. A. Clarke

We present the discovery of several Ultra Compact Dwarfs (UCDs) located in field/group environments. Examination of these objects, plus literature objects, confirms the existence of two distinct formation channels for UCDs. We find that the…

宇宙学与河外天体物理 · 物理学 2015-05-27 Mark A. Norris , Sheila J. Kannappan

We use HST/ACS imaging of 100 early-type galaxies in the ACS Virgo Cluster Survey to investigate the nature of diffuse star clusters (DSCs). Compared to globular clusters (GCs), these star clusters have moderately low luminosities (M_V >…

We present a novel approach to constrain the formation channels of Ultra-Compact Dwarf Galaxies (UCDs). This inhomogeneous class of objects of remnants of tidally stripped dwarf elliptical galaxies and high mass globular clusters. We use…

星系天体物理 · 物理学 2016-02-03 Karina Voggel , Michael Hilker , Tom Richtler

We make use of the unprecedented depth, spatial resolution, and field of view of the Euclid Early Release Observations of the Perseus galaxy cluster to detect and characterise the dwarf galaxy population in this massive system. The Euclid…

星系天体物理 · 物理学 2025-04-30 F. R. Marleau , J. -C. Cuillandre , M. Cantiello , D. Carollo , P. -A. Duc , R. Habas , L. K. Hunt , P. Jablonka , M. Mirabile , M. Mondelin , M. Poulain , T. Saifollahi , R. Sánchez-Janssen , E. Sola , M. Urbano , R. Zöller , M. Bolzonella , A. Lançon , R. Laureijs , O. Marchal , M. Schirmer , C. Stone , A. Boselli , A. Ferré-Mateu , N. A. Hatch , M. Kluge , M. Montes , J. G. Sorce , C. Tortora , A. Venhola , J. B. Golden-Marx , N. Aghanim , A. Amara , S. Andreon , N. Auricchio , M. Baldi , A. Balestra , S. Bardelli , P. Battaglia , R. Bender , C. Bodendorf , E. Branchini , M. Brescia , J. Brinchmann , S. Camera , G. P. Candini , V. Capobianco , C. Carbone , J. Carretero , S. Casas , M. Castellano , S. Cavuoti , A. Cimatti , G. Congedo , C. J. Conselice , L. Conversi , Y. Copin , F. Courbin , H. M. Courtois , M. Cropper , A. Da Silva , H. Degaudenzi , A. M. Di Giorgio , J. Dinis , M. Douspis , C. A. J. Duncan , X. Dupac , S. Dusini , A. Ealet , M. Farina , S. Farrens , S. Ferriol , P. Fosalba , S. Fotopoulou , M. Frailis , E. Franceschi , M. Fumana , S. Galeotta , B. Garilli , W. Gillard , B. Gillis , C. Giocoli , P. Gómez-Alvarez , A. Grazian , F. Grupp , L. Guzzo , M. Hailey , S. V. H. Haugan , J. Hoar , H. Hoekstra , W. Holmes , I. Hook , F. Hormuth , A. Hornstrup , D. Hu , P. Hudelot , K. Jahnke , M. Jhabvala , E. Keihänen , S. Kermiche , A. Kiessling , T. Kitching , R. Kohley , B. Kubik , K. Kuijken , M. Kümmel , M. Kunz , H. Kurki-Suonio , O. Lahav , D. Le Mignant , S. Ligori , P. B. Lilje , V. Lindholm , I. Lloro , D. Maino , E. Maiorano , O. Mansutti , O. Marggraf , K. Markovic , N. Martinet , F. Marulli , R. Massey , S. Maurogordato , H. J. McCracken , E. Medinaceli , S. Mei , Y. Mellier , M. Meneghetti , E. Merlin , G. Meylan , M. Moresco , L. Moscardini , E. Munari , R. Nakajima , R. C. Nichol , S. -M. Niemi , C. Padilla , S. Paltani , F. Pasian , K. Pedersen , W. J. Percival , V. Pettorino , S. Pires , G. Polenta , M. Poncet , L. A. Popa , L. Pozzetti , F. Raison , R. Rebolo , A. Refregier , A. Renzi , J. Rhodes , G. Riccio , H. -W. Rix , E. Romelli , M. Roncarelli , E. Rossetti , R. Saglia , D. Sapone , R. Scaramella , P. Schneider , A. Secroun , G. Seidel , M. Seiffert , S. Serrano , C. Sirignano , G. Sirri , L. Stanco , P. Tallada-Crespí , A. N. Taylor , H. I. Teplitz , I. Tereno , R. Toledo-Moreo , A. Tsyganov , I. Tutusaus , E. A. Valentijn , L. Valenziano , T. Vassallo , G. Verdoes Kleijn , A. Veropalumbo , Y. Wang , J. Weller , O. R. Williams , G. Zamorani , E. Zucca , C. Baccigalupi , A. Biviano , C. Burigana , G. De Lucia , K. George , V. Scottez , M. Viel , P. Simon , A. Mora , J. Martín-Fleitas , D. Scott