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Related papers: NGC 4340: Double Bar + Fossil Nuclear Ring

200 papers

We present a detailed study of the peculiar HI-deficient Virgo cluster spiral galaxies NGC 4064 and NGC 4424, using $^{12}$CO 1-0 interferometry, optical imaging and integral-field spectroscopic observations, in order to learn what type of…

Astrophysics · Physics 2008-11-26 J. R. Cortes , J. D. P. Kenney , E. Hardy

NGC 3642 was classified as a spiral galaxy with three rings and no bar. We have performed an HI and optical study of this nearly face-on galaxy. We find that the nuclear ring might in fact be part of an inner one-armed spiral, that could be…

Astrophysics · Physics 2009-11-07 L. Verdes--Montenegro , A. Bosma , E. Athanassoula

{\it Hubble Space Telescope} (\hst) Wide Field Planetary Camera 2 ({\it WFPC2}) images of the Virgo Cluster dwarf elliptical galaxy VCC 128 reveal an apparently double nucleus. The two components, which are separated by $\sim 32$ pc in…

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…

Double-barred galaxies are common in the local Universe, with approximately one third of barred spirals hosting an smaller, inner bar. Nested bars have been proposed as a mechanism for transporting gas to the very central regions of the…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-03 A. de Lorenzo-Cáceres , A. Vazdekis , J. A. L. Aguerri , E. M. Corsini , Victor P. Debattista

We describe the results of our spectroscopy for a sample of barred galaxies whose inner regions exhibit an isophotal twist commonly called a secondary bar. The line-of-sight velocity fields of the ionized gas and stars and the…

Astrophysics · Physics 2009-11-07 A. V. Moiseev

We present results from an imaging survey of an unbiased sample of thirty-eight early-type (S0--Sa), low-inclination, optically barred galaxies in the field. Our goal was to find and characterize central stellar and gaseous structures:…

Astrophysics · Physics 2008-11-26 Peter Erwin , Linda S. Sparke

The late-type galaxy NGC 4303 (M61) is one of the most intensively studied barred galaxies in the Virgo Cluster. Its prominent enhanced star formation throughout large areas of the disk can be nicely studied due to its low inclination of…

Astrophysics · Physics 2007-05-23 D. Tsch"oke , G. Hensler , N. Junkes

The mid infrared emission of early type galaxies traces the presence of intermediate age stellar populations as well as even tiny amounts of ongoing star formation. Here we discuss high S/N Spitzer IRS spectra of a sample of Virgo early…

Astrophysics · Physics 2009-11-13 A. Bressan , P. Panuzzo , O. Vega , L. Buson , M. Clemens , G. L. Granato , R. Rampazzo , L. Silva , J. R. Valdes

A remarkable structure is observed in the innermost regions of the barred galaxy NGC 1415 : a small stellar bar, bright circumnuclear ionized gas seen in Halpha, two bright ionized gas sources, seen in Halpha, just beyond the ends of the…

Astrophysics · Physics 2016-08-30 J. A. Garcia-Barreto , E. Moreno

We performed SPH simulations to study the nuclear morphology of a barred galaxy NGC 4314. We have constructed the mass models based on the results of a profile decomposition into disk, bulge, and bar components. Our models have three…

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

Double bars have been proposed as a means of transporting molecular gas past inner Lindblad resonances into the nuclear regions, where it can fuel active or starburst nuclei. Thus far, the existence of double bars has been determined…

Astrophysics · Physics 2009-11-07 Glen Petitpas , Christine Wilson

We present a detailed study of the centre of NGC4654, a Milky Way-like spiral galaxy in the Virgo cluster that has been reported to host a double stellar nucleus, thus promising a rare view of ongoing star cluster infall into a galaxy…

Strongly noncircular outer stellar disks have been found in two unbarred SA0 galaxies by analyzing spectroscopic data on the rotation of stars and photometric data on the shape and orientation of the isophotes. In NGC 502, the oval…

Astrophysics of Galaxies · Physics 2016-11-03 Olga K. Sil'chenko

NGC 4449 is a nearby Magellanic irregular starburst galaxy with a B-band absolute magnitude of -18 and a prominent, massive, intermediate-age nucleus at a distance from Earth of 3.8 megaparsecs. It is wreathed in an extraordinary neutral…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-04 R. M. Rich , M. L. M. Collins , C. M. Black , F. M. Longstaff , A. Koch , A. Benson , D. B. Reitzel

I present a brief review of what is known about double-barred galaxies, where a small ("inner") bar is nested inside a larger ("outer") bar; the review is focused primarily on their demographics and photometric properties. Roughly 20% of…

Cosmology and Nongalactic Astrophysics · Physics 2009-08-07 Peter Erwin

We have made observations of the \ion{H}{1} in the southern ringed barred spiral galaxies NGC~1433 and NGC~6300 with the Australia Telescope Compact Array (ATCA), the main goal being to test the resonance theory for the origin of these…

Here we present the preliminary results of the analysis of VIMOS observations of the central 4.5 kpc of the double-barred galaxy NGC 5850. We use optical diagnostic diagrams to study the main ionization mecahnism across the field of view…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-04 M. Bremer , J. Scharwächter , A. Eckart , J. Zuther , S. Fischer , M. Valencia-S

Galaxies with nuclear bars are believed to efficiently drive gas inward, generating a nuclear starburst and possibly an active galactic nucleus (AGN). We confirm this scenario for the isolated, double-barred, luminous infrared galaxy ESO…

We present near-infrared VLT ISAAC imaging and spectroscopy of the peculiar Virgo galaxy NGC 4438, whose nucleus has been classified as a LINER. The data are supplemented by mid-infrared imaging, and compared to previous WFPC2 HST broadband…

Astrophysics of Galaxies · Physics 2015-05-14 Sebastian Perez , Simon Casassus , Juan R. Cortes , J. D. P. Kenney