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Direct observational evidence for the creation of nuclear star clusters (NSCs) is needed to support the proposed scenarios for their formation. We analysed the dwarf galaxy UGC 7346, located in the peripheral regions of the Virgo Cluster,…

Astrophysics of Galaxies · Physics 2023-03-15 J. Román , P. M. Sánchez-Alarcón , J. H. Knapen , R. Peletier

As a well-known open cluster, NGC 2323 (also called M50) has been widely investigated for over a hundred years and has always been considered a classical single cluster. In this work, with the help of Gaia DR3, we study the binary structure…

We have used the WFPC2 camera of the Hubble Space Telescope to obtain deep F814W images of a blank field in the Virgo Cluster located 41 arcmin northwest of M87. We perform star counts in that field, and in another Virgo field observed by…

We present spatial and spectral results of ROSAT observations of two galaxies: NGC 4569 and NGC 4303. Both objects are members of the Virgo Cluster and have nearby smaller companions with which they have probably gone through an encounter.…

Astrophysics · Physics 2007-05-23 D. Tschoeke , G. Hensler

We performed long-slit spectral observations of two SB-type galaxies: NGC 5347, UGC 1344. They were previously suspected as the galaxies with unusually low mass-to-light ratios (on the ground of mass estimates from the Hi linewidths), which…

Astrophysics of Galaxies · Physics 2017-06-28 A. S. Saburova , I. Yu. Katkov , S. A. Khoperskov , A. V. Zasov , R. I. Uklein

The bright Magellanic irregular galaxy NGC 4449 was observed during the Astro-2 Space Shuttle mission by the Ultraviolet Imaging Telescope (UIT), which obtained images of a ~40 arcmin field centered on the galaxy in two broad…

We report new radio continuum observations with an angular resolution of 2''.1 at 1.4 GHz and 0''.28 at 8.4 GHz of the barred galaxy NGC 3367. In the map at 1.4 GHz the central nuclear region connects to the SW lobe, with a projected…

Astrophysics · Physics 2009-11-07 J. Antonio Garcia-Barreto , Jose Franco , Larry Rudnick

The current picture of galaxy evolution advocates co-evolution of galaxies and their nuclear massive black holes (MBHs), through accretion and merging. Quasar pairs (6,000-300,000 light-years separation) exemplify the first stages of this…

Cosmology and Nongalactic Astrophysics · Physics 2011-09-05 G. Fabbiano , Wang Junfeng , M. Elvis , G. Risaliti

We used a set of moderately-deep and high-resolution optical observations obtained with the Hubble Space Telescope to investigate the properties of the stellar population in the heavily obscured bulge globular cluster NGC 6256. The analysis…

M84 is a giant elliptical galaxy located in the Virgo cluster. Prior imaging with the Hubble Space Telescope (HST) revealed a small, highly inclined, nuclear ionized gas disk, the kinematics of which indicate the presence of a 0.4 -1.5…

Cosmology and Nongalactic Astrophysics · Physics 2010-08-26 Nick Devereux , Michael Eracleous , Paul Hriljac , Andrew Shearer

We present interferometric observations of CO J=1-0 emission in the central regions of the edge-on galaxy NGC 4631, known for its extended gaseous halo and its tidal interactions. Previous single-dish observations revealed that almost all…

Astrophysics · Physics 2009-10-31 Richard J. Rand

NGC 4395 is one of the least luminous and nearest known type 1 Seyfert galaxies, and it also lacks a bulge. We present an HST I-band image of its nuclear region and Keck high-resolution (8 km/s) echelle spectra containing the Ca II…

Astrophysics · Physics 2010-04-06 Alexei V. Filippenko , Luis C. Ho

We present an investigation into the origins of a series of interlaced narrow filamentary stellar structures, loops and plumes in the vicinity of the Virgo Cluster, edge-on spiral galaxy, NGC 4216 that were previously identified by the…

We present {\it Gemini} longslit optical spectroscopy and VLA radio observations of the nuclear region of NGC 4178, a late-type bulgeless disk galaxy recently confirmed to host an AGN through infrared and X-ray observations. Our…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-17 Nathan Secrest , Shobita Satyapal , Sean Moran , Teddy Cheung , Marcello Giroletti , Mario Gliozzi , Marcel Bergmann , Anil Seth

We present CO interferometer observations of the barred galaxy NGC 4303 (M61). This galaxy has a gas concentration at the central region and offset ridges in the bar. Sharp velocity gradients are apparent across the ridges. Analyses of the…

Astrophysics · Physics 2015-06-24 J. Koda , Y. Sofue

We present the results of the stellar and ionized gas kinematics of 13 bright peculiar Virgo cluster galaxies. The stellar velocity field are mostly consistent with a rotation pattern, but some of them shows interesting features such as;…

Astrophysics · Physics 2007-05-23 Juan R. Cortes , Jeffrey D. P. Kenney , Eduardo Hardy

Fornax 4 is the most distinctive globular cluster in the Fornax dwarf spheroidal. Located close to the centre of the galaxy, more metal-rich and potentially younger than its four companions (namely, Fornax clusters number 1, 2, 3 and 5), it…

Solar and Stellar Astrophysics · Physics 2020-06-10 S. Martocchia , E. Dalessandro , M. Salaris , S. Larsen , M. Rejkuba

We report the discovery of diffuse far-infrared and far-ultraviolet emission projected near the interacting pair NGC4435/4438, in the Virgo cluster. This feature spatially coincides with a well known low surface-brightness optical plume,…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-14 L. Cortese , G. J. Bendo , K. G. Isaak , J. I. Davies , B. R. Kent

We present X-ray spectroscopic and morphological analyses using Chandra ACIS and ROSAT observations of the giant elliptical galaxy NGC 4472 in the Virgo cluster. We discuss previously unobserved X-ray structures within the extended galactic…

Astrophysics · Physics 2009-11-10 B. A. Biller , C. Jones , W. R. Forman , R. Kraft , T. Ensslin

We report the discovery of a ring-like cluster complex in the starburst galaxy NGC 2146. The Ruby Ring, so named due to its appearance, shows a clear ring-like distribution of star clusters around a central object. It is located in one of…

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