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Related papers: Nuclear kpc-sized disks of spiral galaxies

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The presence of nuclear discs in barred disc galaxies has been demonstrated in studies on stellar structures and kinematics. It is thus imperative to establish their fundamental properties and scaling relations, which can help understanding…

Astrophysics of Galaxies · Physics 2025-09-19 Dimitri A. Gadotti , Camila de Sá-Freitas

We present photometric and morphological analyses of nuclear star clusters (NSCs) -- very dense, massive star clusters present in the central regions of most galaxies -- in a sample of 33 massive disk galaxies within 20 Mpc, part of the…

Recent high-resolution observations indicate that nuclear spirals are often present in the innermost few hundred parsecs of disc galaxies. My models show that nuclear spirals form naturally as a gas response to non-axisymmetry in the…

Astrophysics · Physics 2007-05-23 Witold Maciejewski

Nuclear spirals can provide a wealth of information about the nuclear potential in disc galaxies. They form naturally as a gas response to non-axisymmetry in the gravitational potential, even if the degree of this asymmetry is very small.…

Astrophysics · Physics 2009-11-10 Witold Maciejewski

We summarize some recent results from our observational campaign to study the central regions of spiral galaxies of late Hubble type (Scd - Sm). These disk-dominated, bulgeless galaxies have an apparently uneventful merger history. The…

We describe the history and results of our study of early-type disk galaxies with the Multi-Pupil Spectrograph of the 6m telescope (MPFS). With the new data we confirm the discovery of chemically distinct nuclei reported in 1992; now such…

Astrophysics · Physics 2007-05-23 Olga K. Silchenko

We analyze formation of grand-design two-arm spiral structure in the nuclear regions of disk galaxies. Such morphology has been recently detected in a number of objects using high-resolution near-infrared observations. Motivated by the…

Astrophysics · Physics 2009-10-31 Peter Englmaier , Isaac Shlosman

In this paper we demonstrate the possibility of inferring the presence of Keplerian gaseous disks using optical ground-based telescopes properly equipped. We have modeled the peculiar bidimensional shape of the emission lines in a sample of…

Astrophysics · Physics 2009-10-30 F. Bertola , M. Cappellari , J. G. Funes , E. M. Corsini , A. Pizzella , J. C. Vega Beltran

Using HST, we identify circumnuclear ($100$-$500$ pc scale) structures in nine new H$_2$O megamaser host galaxies to understand the flow of matter from kpc-scale galactic structures down to the supermassive black holes (SMBHs) at galactic…

Astrophysics of Galaxies · Physics 2017-08-07 Patryk Pjanka , Jenny E. Greene , Anil C. Seth , James A. Braatz , Christian Henkel , Fred K. Y. Lo , Ronald Laesker

The shape of a cusped galactic nucleus is constrained by the range of shapes of orbits in its gravitational potential. It is shown for scale-free non-axisymmetric discs that while a plausible elongated density model requires at least some…

Astrophysics · Physics 2009-10-31 HongSheng Zhao , Marcella Carollo , Tim de Zeeuw

In this paper, the third of a series dedicated to the investigation of the nuclear properties of spiral galaxies, we have (i) modelled the WFPC2 F606W nuclear surface brightness profiles of 41 spiral galaxies presented in Carollo et al.…

Astrophysics · Physics 2009-10-30 C. M. Carollo , M. Stiavelli

We report evidence for nuclear stellar disks in 3 early-type spirals, namely NGC 1425, NGC 3898 and NGC 4698, revealed by WFPC2/F606W images out of a sample of 38 spiral galaxies, selected from the Hubble Space Telescope Data Archive.…

Astrophysics · Physics 2009-11-07 A. Pizzella , E. M. Corsini , L. Morelli , M. Sarzi , C. Scarlata , M. Stiavelli , F. Bertola

Hubble Space Telescope observations of the central kiloparsec of AGN have revealed a wealth of structure, particularly nuclear bars and spirals, that are distinct from analogous features in the disks of spiral galaxies. WFPC2 and NICMOS…

Astrophysics · Physics 2007-05-23 Paul Martini

Hubble Space Telescope images of two early-type galaxies harboring both nuclear and outer stellar discs are studied in detail. By means of a photometric decomposition, the images of NGC 4342 and NGC 4570 are analyzed and the photometric…

Astrophysics · Physics 2009-10-30 Cecilia Scorza , Frank C. van den Bosch

The innermost regions of most galaxies are characterised by the presence of extremely dense nuclear star clusters. Nevertheless, these clusters are not the only stellar component present in galactic nuclei, where larger stellar structures…

We investigate the structural properties of nuclear star clusters in late-type spiral galaxies. More specifically, we fit analytical models to HST images of 39 nuclear clusters in order to determine their effective radii after correction…

The early-type spiral NGC 4698 is known to host a nuclear disc of gas and stars which is rotating perpendicularly with respect to the galaxy main disc. In addition, the bulge and main disc are characterised by a remarkable geometrical…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-04 E. M. Corsini , J. Méndez-Abreu , N. Pastorello , E. Dalla Bontà , L. Morelli , A. Beifiori , A. Pizzella , F. Bertola

We have obtained HST_NICMOS images for 72 nearby spiral galaxy bulges in the H-band. These data show that galaxies with regular bulges have steeper nuclear cusps than galaxies with irregular bulges. We also show that galaxies with regular…

Astrophysics · Physics 2007-05-23 M. Seigar

We report the detection of the Galactic nuclear disc in line-of-sight kinematics of stars, measured with infrared spectroscopy from APOGEE. This stellar component of the nuclear disc has an extent and rotation velocity V ~ 120kms comparable…

Astrophysics of Galaxies · Physics 2015-10-21 Ralph Schönrich , Michael Aumer , Stuart E. Sale

Observations with the Hubble Space Telescope reveal an irregular network of dust spiral arms in the nuclear region of the interacting disk galaxy NGC 2207. The spirals extend from ~50 pc to ~300 pc in galactocentric radius, with a projected…

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