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Related papers: B/PS bulges in DESI Legacy edge-on galaxies I: Sam…

200 papers

We investigate whether the formation mechanism of boxy and peanut-shaped (B/PS) bulges could depend on the gas content of the galaxy. We have performed N-body simulations with and without a gaseous component. In the second case star…

Astrophysics of Galaxies · Physics 2009-02-06 Herve Wozniak , Leo Michel-Dansac

To investigate galaxy properties as a function of their total stellar mass, we obtained 21cm HI line observations at the 100-m class Nan\c{c}ay Radio Telescope of 2839 galaxies from the Sloan Digital Sky Survey (SDSS) in the Local Volume…

We examine the effects that the modelling of a Boxy/Peanut (B/P) bulge will have on the estimates of the stellar gravitational potential, forces, orbital structure and bar strength of barred galaxies. We present a method for obtaining the…

Astrophysics of Galaxies · Physics 2015-06-24 F. Fragkoudi , E. Athanassoula , A. Bosma , F. Iannuzzi

We use detailed modeling of stellar populations of nearby galaxies to calculate population parameters. Our sample of galaxies includes most galaxies of the Local Group and several more distant giant galaxies. Available data are sufficient…

Astrophysics · Physics 2007-05-23 J. Einasto , P. Tenjes

We present a two-dimensional multi-component photometric decomposition of 404 galaxies from the CALIFA Data Release 3. They represent all possible galaxies with no clear signs of interaction and not strongly inclined in the final CALIFA…

We have used the EFAR sample of galaxies to study the light distributions of early-type galaxies. We decompose the 2D light distribution of the galaxies in a flattened spheroidal component with a Sersic radial light profile and an inclined…

In this paper I present a new two-dimensional decomposition technique, which models the surface photometry of a galaxy with an exponential light profile for both bulge and disk and, when necessary, with a Freeman bar. The new technique was…

Astrophysics · Physics 2007-05-23 Roelof S. de Jong

Bulge-disk (B-D) decomposition is an effective diagnostic to characterize the galaxy morphology and understand its evolution across time. So far, high-quality data have allowed detailed B-D decomposition to redshift below 0.5, with limited…

We investigate the scaling relations of bulge and disk structural parameters for a sample of 108 disk galaxies.Structural parameters are obtained from 2D bulge/disk decomposition of H-band images.Bulges are modelled with a generalized…

Astrophysics · Physics 2009-11-10 L. K. Hunt , D. Pierini , C. Giovanardi

We present an analysis of the evolution of the central mass-density profile of massive elliptical galaxies from the SLACS and BELLS strong gravitational lens samples over the redshift interval z ~ 0.1-0.6, based on the combination of…

We explore the evolution of the stellar mass-size relation of galaxies of different morphological types and specifically bulge and disk components. We use a sample of $\sim35,000$ galaxies within a redshift range $0 < z < 1$, and stellar…

Astrophysics of Galaxies · Physics 2022-05-09 Abdolhosein Hashemizadeh

We perform two-dimensional, Point-Spread-Function-convolved, bulge+disk decompositions in the $g$ and $r$ bandpasses on a sample of 1,123,718 galaxies from the Legacy area of the Sloan Digital Sky Survey Data Release Seven. Four different…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-28 Luc Simard , J. Trevor Mendel , David R. Patton , Sara L. Ellison , Alan W. McConnachie

The formation and evolution of disk-dominated galaxies is difficult to explain, yet these objects exist. We therefore embarked on a study aimed at a better understanding of these enigmatic objects. We used data from the SDSS DR1 in order to…

Astrophysics · Physics 2009-11-11 S. J. Kautsch , E. K. Grebel , F. D. Barazza , J. S. Gallagher

We have obtained long-slit spectroscopy for a sample of 20 early-type barred galaxies to study the influence of bars in the building of galaxy bulges. Line strength indices were measured and used to derive age and metallicity gradients in…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-27 Isabel Perez , Patricia Sanchez-Blazquez

Barred galaxies have interesting morphological features whose presence and properties set constraints on galactic evolution. Here we examine barlenses, i.e. lens-like components whose extent along the bar major axis is shorter than that of…

Astrophysics of Galaxies · Physics 2016-03-01 E. Athanassoula , E. Laurikainen , H. Salo , A. Bosma

We present a new set of multi-million particle SPH simulations of the formation of disk dominated galaxies in a cosmological context. Some of these galaxies are higher resolution versions of the models already described in Governato et al…

Astrophysics · Physics 2008-01-14 F. Governato , L. Mayer , C. Brook

This study investigates the evolution of the star-forming fraction ($F_{\mathrm{sf}}$) of Brightest Cluster Galaxies (BCGs) at $z<0.8$, using the galaxy clusters identified from the Legacy Imaging Surveys from the Dark Energy Spectroscopic…

Astrophysics of Galaxies · Physics 2025-12-04 Shufei Liu , Hu Zou , Jinfu Gou , Weijian Guo , Niu Li , Wenxiong Li , Gaurav Singh , Haoming Song , Jipeng Sui , Xi Tan , Yunao Xiao , Jingyi Zhang , Lu Feng

We present optical (B & R) and infrared (K_s) images and photometry for a sample of 49 extremely late-type, edge-on disk galaxies selected from the Flat Galaxy Catalog of Karenchentsev et al. (1993). Our sample was selected to include…

Astrophysics · Physics 2009-10-31 Julianne J. Dalcanton , Rebecca A. Bernstein

Internal dynamics and kinematics of galaxies have imprints on the line-of-sight velocity distribution~(LOSVD). Gauss-Hermite parametrisation allows one to identify the kinematics features of the system in terms of skewness~($h_3$) and…

Astrophysics of Galaxies · Physics 2023-11-09 Daria Zakharova , Iliya S. Tikhonenko , Natalia Ya. Sotnikova , A. Smirnov

Inspecting all 1224 edge-on disk galaxies larger than 2' in the RC3 on DSS images we have found several galaxies with extraordinary bulges meeting two criteria: They are box shaped and large in respect to the diameters of their galaxies.…

Astrophysics · Physics 2009-11-10 R. Luetticke , M. Pohlen , R. -J. Dettmar
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