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Lenticular galaxies are believed to form by a combination of environmental effects and secular evolution. We study the nearby disc-dominated S0 galaxy NGC 6340 photometrically and spectroscopically to understand the mechanisms of S0…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-13 Igor Chilingarian , Alexandra Novikova , Veronique Cayatte , Francoise Combes , Paola Di Matteo , Anatoly Zasov

We examine the nuclear morphology, kinematics, and stellar populations in nearby S0 galaxy NGC 404 using a combination of adaptive optics assisted near-IR integral-field spectroscopy, optical spectroscopy, and HST imaging. These…

We have used the Wide Field Planetary Camera 2 aboard the Hubble Space Telescope to image the compact star cluster nuclei of the nearby, late-type, low-luminosity spiral galaxies NGC 4395, NGC 4242, and ESO 359-029. We also analyze archival…

NGC 1313 is a bulgeless nearby galaxy, classified as SB(s)d. Its proximity allows high spatial resolution observations. We performed the first detailed analysis of the emission-line properties in the nuclear region of NGC 1313, using an…

Astrophysics of Galaxies · Physics 2017-01-20 R. B. Menezes , J. E. Steiner

We present the results of a wide-field photometric study of the globular cluster (GC) system of the edge-on Sab spiral NGC7814. This is the first spiral to be fully analyzed from our survey of the GC systems of a large sample of galaxies…

Astrophysics · Physics 2009-11-10 K. L. Rhode , S. E. Zepf

Investigation of gaseous and stellar kinematics and of broad-band VRI and narrow-band H-alpha and [NII]6583 images is performed for the central part (R < 4 kpc) of the regular spiral galaxy NGC 2841. We have found emission-line splitting at…

Astrophysics · Physics 2009-10-31 V. L. Afanasiev , O. K. Sil'chenko

NGC 1232 is a face-on spiral galaxy that serves as an excellent laboratory for the study of star formation due to its proximity. Recent studies have revealed interesting features about this galaxy: X-ray observations suggest that it…

Astrophysics of Galaxies · Physics 2020-09-15 Fabiana Lima-Costa , Lucimara P. Martins , Alberto Rodríguez-Ardila , Luciano Fraga

Using the Wide Field Planetary Camera 2 on board the Hubble Space Telescope, we have imaged a luminous young star cluster in the nearby spiral galaxy NGC 6946. The cluster has an absolute visual magnitude M(V)=-13.2, comparable to the…

Astrophysics · Physics 2009-11-06 S. S. Larsen , J. P. Brodie , B. G. Elmegreen , Y. N. Efremov , P. W. Hodge , T. Richtler

The role of environmentally induced gas stripping in driving galaxy evolution in groups remains poorly understood. Here we present extensive Chandra and Very Large Array mosaic observations of the hot and cold interstellar medium within the…

We present large-scale CCD images of a dozen low surface brightness objects in the vicinity of giant Sc galaxy NGC 6946, which have been found recently on POSS-II copies. Six of them: UGC 11583, kk251, kk252, kkr55, kkr56, and kkr59 are…

Astrophysics · Physics 2007-05-23 I. D. Karachentsev , M. E. Sharina , W. K. Huchtmeier

Using the WiFeS integral field spectrograph, we have undertaken a series of observations of star-forming galaxies in Compact Groups. In this first paper dedicated to the project, we present the analysis of the spiral galaxy NGC838, a member…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-15 Frédéric P. A. Vogt , Michael A. Dopita , Lisa J. Kewley

We have conducted a $UBVRI$ and $H_{\alpha}$ CCD photometry of 5 barred galaxies, NGC 2523, NGC 2950, NGC 3412, NGC 3945 and NGC 5383, along with SPH simulations, in order to understand the origin of young stellar populations in the nuclei…

Astrophysics · Physics 2009-11-07 H. B. Ann

The edge-on Sc galaxy NGC 5907 has been observed in the 12CO(1-0)-line emission using the Nobeyama 45-m telescope. The radial density distribution between 2 and 13 kpc is well represented by a superposition of an exponential-law disk of…

Astrophysics · Physics 2007-05-23 Yoshiaki SOFUE

Most galaxies in the Universe are found in groups, which have various morphologies and dynamical states. Studying how groups evolve is an important step for our understanding in both large-scale structure formation and galaxy evolution. We…

Astrophysics of Galaxies · Physics 2025-05-21 G. B. Lima Neto , H. V. Capelato , F. Durret , R. E. G. Machado

This paper focuses on NGC 1533 and the pair IC 2038 and IC 2039 in Dorado a nearby, clumpy, still un-virialized group. We obtained their surface photometry from deep OmegaCAM@ESO-VST images in g and r bands. For NGC 1533, we map the surface…

We report a galaxy group candidate HPC1001 at $z\approx3.7$ in the COSMOS field. This structure was selected as a high galaxy overdensity at $z>3$ in the COSMOS2020 catalog. It contains ten candidate members, of which eight are assembled in…

We present new narrow-band filter imagery in H-alpha and [N II] 6584 along with UV and optical spectrophotometry measurements from 1200 to 9600 Angstroms of NGC 7293, the Helix Nebula, a nearby, photogenic planetary nebula of large diameter…

Astrophysics · Physics 2009-10-31 R. B. C. Henry , K. B. Kwitter , R. J Dufour

We present the results of the spectral investigation of the regular Sb galaxy NGC 7331 with the Multi-Pupil Field Spectrograph of the 6m telescope. The absorption-line indices H-beta, Mgb, and <Fe> are mapped to analyse the properties of…

Astrophysics · Physics 2009-10-31 Olga K. Sil'chenko

Aims: We present the first in-depth study of the kinematic properties and derive the structural parameters of NGC 4372 based on the fit of a Plummer profile and a rotating, physical model. We explore the link between internal rotation to…

Dorado is a nearby (17.69 Mpc) strongly evolving galaxy group in the Southern Hemisphere. We are investigating the star formation in this group. This paper provides a FUV imaging of NGC 1533, IC 2038 and IC 2039, which form a substructure,…

Astrophysics of Galaxies · Physics 2021-06-23 R. Rampazzo , P. Mazzei , A. Marino , L. Bianchi , S. Ciroi , E. V. Held , E. Iodice , J. Postma , E. Ryan-Weber , M. Spavone , M. Uslenghi