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相关论文: A globular cluster in the dwarf galaxy Sextans B

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We report the confirmation of an old, metal-poor globular cluster in the nearby dwarf irregular galaxy Sextans A, the first globular cluster known in this galaxy. The cluster, which we designate as Sextans A-GC1, lies some 4.4 arcminutes…

The Fornax dwarf spheroidal galaxy has an anomalous number of globular clusters, five, for its stellar mass. There is a longstanding debate about a potential sixth globular cluster (Fornax~6) that has recently been `rediscovered' in DECam…

The chemical composition of globular clusters (GCs) across the Local Group provides information on chemical abundance trends. The host galaxy, Sextans A, is a low-surface-brightness dwarf irregular galaxy located on the edge of the Local…

We report a possible discovery of a relic star cluster in the Sextans dwarf spheroidal galaxy. Using the \textit{hk} index ($\equiv$($Ca-b$)$-$($b-y$)) as a photometric metallicity indicator, we discriminate the metal-poor and metal-rich…

星系天体物理 · 物理学 2019-01-10 Hak-Sub Kim , Sang-Il Han , Seok-Joo Joo , Hyunjin Jeong , Suk-Jin Yoon

We present the results of moderate resolution spectroscopy for a globular cluster in the M81 group dwarf spheroidal galaxy DDO~78. The DDO78 globular cluster, 4 Milky Way globular clusters, spectroscopic and radial velocity standards were…

天体物理学 · 物理学 2009-11-07 M. E. Sharina , O. K. Sil'chenko , A. N. Burenkov

Globular clusters (GCs) are important tools to rebuild the accretion history of a galaxy. There are newly discovered GCs in the Sagittarius (Sgr) dwarf galaxy, that can be used as probes of the accretion event onto the Milky Way (MW). Our…

星系天体物理 · 物理学 2021-10-04 E. R. Garro , D. Minniti , M. Gómez , J. Alonso-García

We have obtained V and I images of the lone globular cluster that belongs to the dwarf Local Group irregular galaxy known as WLM. The color-magnitude diagram of the cluster shows that it is a normal old globular cluster with a well-defined…

天体物理学 · 物理学 2009-10-31 Paul W. Hodge , Andrew E. Dolphin , Toby R. Smith , Mario Mateo

We present the results of medium-resolution spectroscopy of 28 globular clusters (GCs) in six nearby galaxies of different luminosities and morphological types, situated in: M33 (15 objects), M31 (3), IC10 (4), UGCA86 (4), HolmbergIX (1),…

宇宙学与河外天体物理 · 物理学 2015-05-18 Margarita E. Sharina , Rupali Chandar , Thomas H. Puzia , Paul Goudfrooij , Emmanuel Davoust

We present a detailed study of the stellar and HI structure of the dwarf irregular galaxies SextansA and SextansB, members of the NGC3109 association. We use newly obtained deep (r~26.5) and wide field g,r photometry to extend the Surface…

星系天体物理 · 物理学 2014-07-02 M. Bellazzini , G. Beccari , F. Fraternali , T. A. Oosterloo , A. Sollima , V. Testa , S. Galleti , S. Perina , M. Faccini , F. Cusano

We present tentative evidence for the existence of a dissolved star cluster in the Sextans dwarf spheroidal galaxy. In a sample of six stars, we identify three (possibly four) stars around [Fe/H] =-2.7 that are highly clustered in a…

宇宙学与河外天体物理 · 物理学 2012-02-20 Torgny Karlsson , Joss Bland-Hawthorn

We use Hubble Space Telescope imaging to show that the nearby dwarf starburst galaxy NGC 4449 has an unusual abundance of luminous red star clusters. Joint constraints from integrated photometry, low-resolution spectroscopy, dynamical…

宇宙学与河外天体物理 · 物理学 2015-06-03 Jay Strader , Anil C. Seth , Nelson Caldwell

We present a comprehensive analysis of the globular cluster (GC) system of the Local Group dwarf irregular galaxy NGC 6822. Our study is based on homogeneous optical and near-IR photometry, as well as long-slit spectroscopic observations…

We present intermediate-resolution (R$\sim$1000) spectra in the $\sim$3500-10,000 A range of 14 globular clusters in the magellanic irregular galaxy NGC 4449 acquired with the Multi Object Double Spectrograph on the Large Binocular…

The spectroscopic and photometric signals of the star-to-star abundance variations found in globular clusters seem to be correlated with global parameters like the cluster's metallicity, mass and age. Understanding this behaviour could…

Recent work on globular cluster systems in dwarf galaxies outside the Local Group is reviewed. Recent large imaging surveys with the Hubble Space Telescope and follow-up spectroscopy with 8-m class telescopes now allow us to compare the…

天体物理学 · 物理学 2007-05-23 Bryan W. Miller

The number of known globular clusters in the Galactic bulge has been increasing steadily thanks to different new surveys. The aim of this study is to provide a census of the newly revealed globular clusters in the Galactic bulge, and…

星系天体物理 · 物理学 2024-08-06 E. Bica , S. Ortolani , B. Barbuy , R. A. P. Oliveira

We present low resolution, integrated Keck spectra of the five globular clusters (GCs) of the Fornax dwarf spheroidal galaxy. We find a tentative age spread among the clusters, with the GC H5 younger by 2-3 Gyr than the others. The clusters…

天体物理学 · 物理学 2009-11-07 Jay Strader , Jean P. Brodie , Duncan A. Forbes , Michael A. Beasley , John P. Huchra

We here present the results of an analysis of the optical spectroscopy of 42 globular cluster (GC) candidates in the nearby spiral galaxy M81 (3.61~Mpc). The spectra were obtained using the long-slit and MOS modes of the OSIRIS instrument…

We present a detailed study of the stellar and HI structure of the dwarf irregular galaxy Sagittarius. We use new deep and wide field photometry to trace the surface brightness profile of the galaxy out to ~5.0' (corresponding to ~1600 pc)…

星系天体物理 · 物理学 2015-06-22 G. Beccari , M. Bellazzini , F. Fraternali , G. Battaglia , S. Perina , A. Sollima , T. A. Oosterloo , V. Testa , S. Galleti
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