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We present the results of the VLT/VIMOS integral-field spectroscopic observations of the inner 28"x28" (3.1 kpc x 3.1 kpc) of the interacting spiral NGC 5719, which is known to host two co-spatial counter-rotating stellar discs. At each…

NGC 6744 is the nearest and brightest south-hemisphere galaxy with a morphological type similar to that of the Milky Way. Using data obtained with the Integral Field Unit of the Gemini South Multi-Object Spectrograph, we found that this…

Astrophysics of Galaxies · Physics 2018-07-10 Patrícia da Silva , J. E. Steiner , R. B. Menezes

We present UBVRI broad band, H$\alpha$ narrow band photometry of the star forming complexes in the infra-red bright galaxy NGC 1084. Results of medium resolution spectroscopy of some of the brighter complexes are also discussed.…

Astrophysics · Physics 2009-11-13 S. Ramya , D. K. Sahu , T. P. Prabhu

(abridged)We present the observations of the pair of interacting galaxies NGC6285/86 carried out with the 6m SAO RAS telescope by using 1D and 2D spectroscopy. The observations of NGC6286 with a long-slit spectrograph (UAGS) near the…

High-spatial resolution near-infrared (NIR) images of the central 24 x 24 arcsec^2 (~ 2 x 2 kpc^2) of the elliptical galaxy NGC 1052 reveal a total of 25 compact sources randomly distributed in the region. Fifteen of them exhibit Halpha…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-20 J. A. Fernández-Ontiveros , C. López-Sanjuan , M. Montes , M. A. Prieto , J. A. Acosta-Pulido

We report the discovery of a transparent sightline at projected distances of {\rho} < 20 kpc to an interacting pair of mature galaxies at z = 0.12. The sightline of the UV-bright quasar PG1522+101 at z = 1.328 passes at {\rho} = 11.5 kpc…

Astrophysics of Galaxies · Physics 2015-06-18 Sean D. Johnson , Hsiao-Wen Chen , John S. Mulchaey , Todd M. Tripp , J. Xavier Prochaska , Jessica K. Werk

Nearby merging pairs are unique laboratories in which one can study the gravitational effects on the individual interacting components. In this manuscript, we report the characterization of selected HII regions along the peculiar galaxy NGC…

We present a discovery of a giant stellar halo in NGC 6822, a dwarf irregular galaxy in the Local Group. This halo is mostly made of old red giants, showing striking features: 1) it is several times larger than the main body of the galaxy…

Astrophysics · Physics 2009-11-11 Myung Gyoon Lee , Narae Hwang

We present results from our Giant Metrewave Radio Telescope (GMRT) HI, Himalayan Chandra Telescope (HCT) Halpha, 1m Sampurnanand Telescope (ST) and 1.3m Devasthal Fast Optical Telescope (DFOT) deep optical observations of NGC 7805/6 (Arp…

We present the line observations in our ALMA imaging spectral scan toward three deeply buried nuclei in NGC 4418 and Arp 220. We cover 67 GHz in $f_{\rm rest}$=215-697 GHz at about 0.2$"$ (30, 80 pc) resolution. All the nuclei show dense…

Astrophysics of Galaxies · Physics 2022-01-05 Kazushi Sakamoto , Sergio Martin , David J. Wilner , Susanne Aalto , Aaron S. Evans , Nanase Harada

Multi-band images of the very isolated spiral galaxy NGC 5523 show a number of unusual features consistent with NGC 5523 having experienced a significant merger: (1) Near-infrared (NIR) images from the Spitzer Space Telescope (SST) and the…

Astrophysics of Galaxies · Physics 2017-02-15 Leah M. Fulmer , John S. Gallagher , Ralf Kotulla

We present HST WFPC2 observations, supplemented by ground-based H-alpha data, of the star-cluster populations in two pairs of interacting galaxies, selected for being in very different kinds of encounters seen at different stages. Dynamical…

Astrophysics · Physics 2009-11-10 William C. Keel , Kirk D. Borne

The typical galaxy in the local universe is expected to be in a self-regulated quasi-equilibrium, displaying a settled morphology that falls within the Hubble Sequence. The Arp and Arp-Madore catalogs are filled with striking examples of…

Astrophysics of Galaxies · Physics 2025-09-12 Julianne J. Dalcanton , Meredith J. Durbin , Benjamin F. Williams

The galaxy NGC1313 has attracted the attention of various studies due to the peculiar morphology observed in optical bands, although it is classified as a barred, late-type galaxy with no apparent close-by companions. However, the velocity…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-04 Esteban Silva-Villa , Soeren Larsen

Globular clusters (GCs) are fundamental tools to unveil the interaction and merger history of their host galaxies. Our goal is to perform the photometric analysis of the globular cluster system (GCS) of the elliptical galaxy NGC 4709, which…

Astrophysics of Galaxies · Physics 2025-08-28 S. Federle , M. Gómez , S. Mieske , F. Dux , M. Hilker , I. A. Yegorova

We examine the merger stage of IRAS 03158+4227, one of the most luminous ULIRGs from the IRAS 2 Jy sample. Deep optical images are presented along with high-resolution NIR images and optical low-resolution spectra. IRAS 03158+4227 is…

Astrophysics · Physics 2009-11-07 H. Meusinger , B. Stecklum , Ch. Theis , J. Brunzendorf

We have discovered three globular clusters beyond the Holmberg radius in Hubble Space Telescope Advanced Camera for Surveys images of the gas-rich dark matter dominated blue compact dwarf galaxy NGC2915. The clusters, all of which start to…

We report on a study of tidally triggered star formation in galaxies, based on spectroscopic/photometric observations in the optical/near-IR of a magnitude limited sample of 59 systems of interacting and merging galaxies and a comparison…

Astrophysics · Physics 2007-05-23 Nils Bergvall , Eija Laurikainen , Susanne Aalto

We study the globular cluster system (GCS) of the giant elliptical NGC4374 (M84) in the Virgo cluster using B and R photometry. The colour distribution is bimodal with peaks at B-R=1.11 and B-R=1.36, fitting well to those found in other…

Astrophysics · Physics 2009-11-10 M. Gomez , T. Richtler

We present the results of B, V, R surface photometry of ESO603-G21 - a galaxy with a possible polar ring. The morphological and photometric features of this galaxy are discussed. The central round object of the galaxy is rather red and…

Astrophysics · Physics 2009-11-07 V. P. Reshetnikov , M. Faundez-Abans , M. de Oliveira-Abans