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The structural parameters of a magnitude-limited sample of 148 unbarred S0-Sb galaxies were derived using the GASP2D algorithm and then analyzed to derive the intrinsic shape of their bulges. We developed a new method to derive the…

宇宙学与河外天体物理 · 物理学 2010-12-30 J. Mendez-Abreu , E. Simonneau , J. A. L. Aguerri , E. M. Corsini

I discuss results from the COSMOS survey, showing that the fraction of disc galaxies that is barred decreases considerably with look-back time from z ~ 0.2 to z ~ 0.8. This decrease is more important for small mass and low luminosity…

天体物理学 · 物理学 2008-02-04 E. Athanassoula

This review summarizes some aspects of the central kiloparsec scale structure of galaxies, and in particular spiral galaxies, elliptical galaxies and merger remnants. The focus is on results from optical and near-IR imaging and…

天体物理学 · 物理学 2007-05-23 Roeland P. van der Marel

Many 3D N-body barred models of the Galaxy extending beyond the Solar circle are realised by self-consistent evolution of various bar unstable axisymmetric models. The COBE/DIRBE K-band map, corrected for extinction, is used to constrain…

天体物理学 · 物理学 2009-10-26 R. Fux

We present the first study of large-scale bars in clusters at intermediate redshifts (z=0.4-0.8). We compare the properties of the bars and their host galaxies in the clusters with those of a field sample in the same redshift range. We use…

宇宙学与河外天体物理 · 物理学 2009-01-30 Fabio D. Barazza , Pascale Jablonka , the EDisCS collaboration

The `Triangal' galaxy evolution schema is used to assess whether the Tuning Fork (bar strength) or the van~den~Bergh Trident and ATLAS$^{3D}$ Comb (spiral strength) offer greater evolutionary insight. A new catalogue of quantitative bar…

星系天体物理 · 物理学 2026-04-28 Alister W. Graham

We construct numerical models of mildly triaxial elliptical galaxies with central density cusps. Using a technique we call ``adiabatic squeezing'', we begin with a spherical gamma=1 Hernquist model and apply a drag to the velocities of the…

天体物理学 · 物理学 2009-10-31 Kelly Holley-Bockelmann , J. Christopher Mihos , Steinn Sigurdsson , Lars Hernquist

Boxy/Peanut/X-shaped (B/P/X) bulges are studied using the 3.6 mum images from the Spitzer Survey of Stellar Structure in Galaxies, and the K_s-band images from the Near-IR S0 galaxy Survey. They are compared with the properties of…

星系天体物理 · 物理学 2014-08-25 E. Laurikainen , H. Salo , E. Athanassoula , A. Bosma , M. Herrera-Endoqui

We present optical broad- and narrow-band imaging of a sample of a dozen barred galaxies. These images are analyzed in conjunction with our previously published near-infrared imaging of their central regions and with literature values for,…

天体物理学 · 物理学 2009-11-07 J. H. Knapen , D. Perez-Ramirez , S. Laine

We present extended stellar kinematics for a sample of 13 elliptical galaxies in the Fornax cluster. Major-axis velocity dispersion profiles (VDPs) and rotation curves (RCs) are given for 12 of the galaxies. A major feature of this data is…

天体物理学 · 物理学 2009-10-30 Alister Graham , Matthew Colless , Giovanni Busarello , Simone Zaggia , G. Longo

Double bars make up a significant fraction of barred galaxies. We propose a new formation scenario for double bars that involves tidal interactions. We demonstrate the viability of this scenario using two examples of simulated galaxies from…

星系天体物理 · 物理学 2023-10-02 Marcin Semczuk , Ewa L. Łokas , Adriana de Lorenzo-Cáceres , E. Athanassoula

As a result of a systematic NIR H-band (1.65 micron) imaging survey of normal galaxies in the local universe, we are able to measure in a highly homogeneous way photometric and structural properties for a sample of 1143 galaxies. We base…

天体物理学 · 物理学 2009-11-07 M. Scodeggio , G. Gavazzi , P. Franzetti , A. Boselli , S. Zibetti , D. Pierini

We present a catalogue of variable stars in the near-infrared wavelength detected with overlapping regions of the 2MASS public images, and discuss their properties. The investigated region is in the direction of the Galactic center (-30 < l…

太阳与恒星天体物理 · 物理学 2014-11-20 Shinjirou Kouzuma , Hitoshi Yamaoka

Numerical simulations have shown that the X-shaped structure in the Milky Way bulge can naturally arise from the bar instability and buckling instability. To understand the influence of the buckling amplitude on the morphology of the…

星系天体物理 · 物理学 2015-12-16 Zhao-Yu Li , Juntai Shen

As a result of our statistical study of 540 edge-on galaxies, we present here the images and preliminary statistical analysis of a sub-sample of 60 galaxies, that were selected to be S-type warped spirals. Computing the average volumic…

天体物理学 · 物理学 2009-10-31 Vladimir Reshetnikov , Francoise Combes

We present results of an analysis of the J, H, and K$_s$ 2MASS images of 139 spiral edge-on galaxies selected from the Revised Flat Galaxies Catalog. The basic structural parameters scalelength (h), scaleheight (z_0), and central surface…

宇宙学与河外天体物理 · 物理学 2015-05-13 Dmitry Bizyaev , Sofia Mitronova

We present optical long-slit and SparsePak Integral Field Unit emission line spectroscopy along with optical broadband and near IR images of the edge-on spiral galaxy NGC 2683. We find a multi-valued, figure-of-eight velocity structure in…

宇宙学与河外天体物理 · 物理学 2015-05-13 Rachel Kuzio de Naray , Matthew J. Zagursky , Stacy S. McGaugh

We present a comprehensive study of bar structures in the local Universe using data from the DESI Legacy Imaging Surveys. Through isophotal analysis of 232,142 galaxies, we identify bars and classify them into strong and weak categories…

星系天体物理 · 物理学 2025-03-31 Wenwen Wang , Zhimin Zhou

Stellar photometry obtained using the Hubble Space Telescope is used to study the distributions of the number densities of stars of various ages in 12 irregular and dwarf spiral galaxies viewed edge-on. Two subsystems can be distinguished…

天体物理学 · 物理学 2007-05-23 N. A. Tikhonov