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Related papers: The isolated interacting galaxy pair NGC 5426/27 (…

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We have determined the structure and kinematics of ionised gas in the weak oval bar of the archetypal Seyfert 1 galaxy, NGC 4151, using the TAURUS Fabry-Perot interferometer to simultaneously map the distribution and kinematics of Hbeta…

Astrophysics · Physics 2009-11-10 M. W. Asif , C. G. Mundell , A. Pedlar

We present fully sampled high angular resolution two-dimensional kinematics in the H alpha spectral line, optical and near-infrared imaging, as well as 21 cm atomic hydrogen data of the spiral galaxy NGC 278. This is a small non-barred…

Astrophysics · Physics 2009-11-10 J. H. Knapen , L. F. Whyte , W. J. G. de Blok , J. M. van der Hulst

We study the comoving relative velocities, v12, of model isolated galaxy pairs at z=0.5. For this purpose, we use the predictions from the GALFORM semi-analytical model of galaxy formation and evolution based on a Lambda cold dark matter…

Cosmology and Nongalactic Astrophysics · Physics 2013-10-01 V. Gonzalez-Perez , E. Jennings , M. -C. Cousinou , S. Escoffier , A. Tilquin , A. Ealet

We present a detailed study of the stellar kinematics in the barred galaxy NGC 5728 based on I-band photometry and long-slit spectroscopic observations in the region of the near-IR Ca II triplet. The analysis of the stellar line-of-sight…

Astrophysics · Physics 2016-08-30 F. Prada , C. M. Gutierrez

We present new observations of the strongly-barred galaxy NGC 1365, including new photometric images and Fabry-Perot spectroscopy, as well as a detailed re-analysis of the neutral hydrogen observations from the VLA archive. We find the…

Astrophysics · Physics 2009-11-13 R. Zanmar Sanchez , J. A. Sellwood , B. J. Weiner , T. B. Williams

The nucleus of the box-shaped galaxy NGC4013 has been observed with the IRAM interferometer in the J=1-0 and J=2-1 lines of 12CO. Our maps show the existence of a fast--rotating(130 km/s) molecular gas disk of radius r=110pc. Several…

Astrophysics · Physics 2008-11-26 S. Garcia-Burillo , F. Combes , R. Neri

We present CO(1-0) and CO(2-1) maps of the interacting barred LINER/Seyfert 2 galaxy NGC 3627 obtained with the IRAM interferometer at resolutions of 2.1" x 1.3" and 0.9" x 0.6", respectively. The molecular gas emission shows a nuclear…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-27 V. Casasola , L. K. Hunt , F. Combes , S. Garcia-Burillo , R. Neri

We present data probing the spatial and kinematical distribution of both the atomic (HI) and molecular (CO) gas in NGC 5218, the late-type barred spiral galaxy in the spiral-elliptical interacting pair, Arp 104. We consider these data in…

Astrophysics · Physics 2008-11-26 H. Cullen , P. Alexander , D. A. Green , K. Sheth

We investigate the atomic and molecular interstellar medium and star formation of NGC 275, the late-type spiral galaxy in Arp 140, which is interacting with NGC 274, an early-type system. The atomic gas (HI) observations reveal a tidal tail…

Astrophysics · Physics 2008-11-26 H. Cullen , P. Alexander , D. A. Green , M. Clemens , K. Sheth

Here we present new measurements of effective radii, surface brightnesses and internal velocity dispersions for 23 isolated early-type galaxies. The photometric properties are derived from new multi-colour imaging of 10 galaxies, whereas…

Astrophysics · Physics 2009-11-11 Fatma M. Reda , Duncan A. Forbes , George K. T. Hau

This paper presents surface photometry (B,V, I, J, H, K) and H_alpha rotation curves of 27 isolated spiral galaxies. The final goal is to obtain the mass distribution of a sample of isolated spiral galaxies in order to model their gas…

Astrophysics · Physics 2009-11-11 I. Perez , I. Marquez , K. Freeman , R. Fux

We present surface photometry and stellar kinematics of IC 3167, a dwarf galaxy hosting a lopsided weak bar and infalling into the Virgo cluster. We measured the bar radius and strength from broad-band imaging and bar pattern speed by…

Astrophysics of Galaxies · Physics 2022-07-20 V. Cuomo , E. M. Corsini , L. Morelli , J. A. L. Aguerri , Y. H. Lee , L. Coccato , A. Pizzella , C. Buttitta , D. Gasparri

In the standard cosmological model of galaxy evolution, mergers and interactions play a fundamental role in shaping galaxies. Galaxies that are currently isolated are thus interesting, allowing us to distinguish between internal and…

We have observed 10 interacting galaxy pairs using the Fabry-Perot interferometer GH$\alpha$FaS (Galaxy H$\alpha$ Fabry-Perot system) on the $4.2\rm{m}$ William Herschel Telescope (WHT) at the Observatorio del Roque de los Muchachos, La…

We measured the bar pattern speed, $\om$, of the SB0 galaxy NGC 1023 using the Tremaine-Weinberg (1984) method with stellar-absorption slit spectroscopy. The morphology and kinematics of the \hi gas outside NGC 1023 suggest it suffered a…

Astrophysics · Physics 2009-11-07 Victor P. Debattista , Enrico Maria Corsini , J. A. L. Aguerri

The velocity field of the nearly face-on galaxy NGC 3631, derived from observations in the H alpha line and the HI radio line, is analysed to study perturbations related to the spiral structure of the galaxy. We confirm our previous…

The galaxy system around NGC4490 was recently highlighted to display a flattened, kinematically correlated structure reminiscent of satellite galaxy planes around other hosts. Since known satellite planes are in tension with $\Lambda$CDM…

We present the stellar and ionized gas kinematics of 13 bright peculiar Virgo cluster galaxies observed with the DensePak Integral Field Unit at the WIYN 3.5-meter telescope, to seek kinematic evidence that these galaxies have experienced…

Astrophysics of Galaxies · Physics 2015-06-23 J. R. Cortés , J. D. P. Kenney , E. Hardy

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 results from {\it Chandra} observations of the galaxy pair NGC 7619 and NGC 7626, the two dominant members of the Pegasus group. The X-ray images show a brightness edge associated with each galaxy, which we identify as merger…

Astrophysics · Physics 2011-02-11 S. W. Randall , C. Jones , R. Kraft , W. R. Forman , E. O'Sullivan