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Related papers: Structure of Disk Dominated Galaxies I. Bulge/Disk…

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Updating Kormendy & Kennicutt (2004, ARAA, 42, 603), we review internal secular evolution of galaxy disks. One consequence is the growth of pseudobulges that often are mistaken for true (merger-built) bulges. Many pseudobulges are…

Astrophysics · Physics 2008-10-16 John Kormendy , David B. Fisher

This paper is the third in a series, studying the optical properties of a sample of mid-IR Warm Seyfert galaxies and of a control sample of mid-IR Cold galaxies. The present paper is devoted to surface photometry. We analyse the light…

Astrophysics · Physics 2007-05-23 Eleni T. Chatzichristou

We present a new database of our two-dimensional bulge-disk decompositions for 14,233 galaxies drawn from SDSS DR12 in order to examine the properties of bulges residing in the local universe ($0.005 < z < 0.05$). We performed…

Astrophysics of Galaxies · Physics 2016-07-20 Keunho Kim , Sree Oh , Hyunjin Jeong , Alfonso Aragon-Salamanca , Rory Smith , Sukyoung K. Yi

We present first results of a program to study the dynamics of undisturbed bulgeless, low surface density disk galaxies in order to probe the underlying structure of dark matter halos. High resolution H-alpha rotation curves are combined…

Astrophysics · Physics 2007-05-23 J. J. Dalcanton , R. A. Bernstein

Structural analysis has been performed for a sample of 15 Southern early-type disk galaxies, mainly S0s, using high resolution $K_s$-band images. The galaxies are mostly barred and many of them show multiple structures including bars and…

Astrophysics · Physics 2009-11-11 E. Laurikainen , H. Salo , R. Buta , J. Knapen , T. Speltincx , D. Block

We have in recent years come to view the outer parts of galaxies as having vital clues about their formation and evolution. Here, we would like to briefly present our results from a complete sample of nearby, late-type, spiral galaxies,…

Astrophysics · Physics 2015-06-24 M. Pohlen , I. Trujillo

We have constructed self-consistent light and mass distribution models for four disk galaxies at redshifts z = 0.48, 0.58, 0.81 and 0.88, using the HST archive WFPC2 observations and rotation curves measured by Vogt et al. (1996) and…

Astrophysics · Physics 2007-05-23 A. Tamm , P. Tenjes

We present one of the largest homogeneous sets of spiral and lenticular galaxy brightness profile decompositions completed to date. The 659 galaxies in our sample have been fitted with a deVaucouleurs' law for the bulge component and an…

Astrophysics · Physics 2009-10-30 W. E. Baggett , S. M. Baggett , K. S. J. Anderson

We present a survey of the mass surface-density of spiral disks, motivated by outstanding uncertainties in rotation-curve decompositions. Our method exploits integral-field spectroscopy to measure stellar and gas kinematics in nearly…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-18 Matthew A. Bershady , Marc A. W. Verheijen , Rob A. Swaters , David R. Andersen , Kyle B. Westfall , Thomas Martinsson

We review internal processes of secular evolution in galaxy disks, concentrating on the buildup of dense central features that look like classical, merger-built bulges but that were made slowly out of disk gas. We call these pseudobulges.…

Astrophysics · Physics 2009-09-29 John Kormendy , Robert C. Kennicutt

For a compiled sample of disk galaxies with available photometry (B and K bands), velocity line-widths and HI integral fluxes, several parameters which trace the luminous, baryonic and dark matter contents were inferred. We investigated how…

Astrophysics · Physics 2009-11-07 J. Zavala , V. Avila-Reese , H. Hernandez-Toledo , C. Firmani

We present evolutionary synthesis models for both components and add their spectra in various proportions to obtain the full range of local galaxies' B-band bulge-to-total light ratios. Bulge star formation is assumed to occur on a short…

Astrophysics · Physics 2009-11-07 Jochen Schulz , Uta Fritze-v. Alvensleben , Klaus J. Fricke

Relying on samples of disk galaxies for which a detailed photometric bulge/disk decomposition has been provided in the literature, we examine the dependence of the bulge-to-disk luminosity ratio (B/D) on the blue absolute luminosity and on…

We have studied a sample of 101 bright 2MASS galaxies from the Large Galaxy Atlas (LGA), whose morphologies span from early to late-types. We have generated estimates for structural parameters through a two-dimensional (2D) surface…

We investigate the evolution of galactic disks in N-body Tree-SPH simulations. We find that disks, initially truncated at three scale-lengths, can triple their radial extent, solely driven by secular evolution. Both Type I (single…

Astrophysics of Galaxies · Physics 2015-06-04 I. Minchev , B. Famaey , A. C. Quillen , P. Di Matteo , F. Combes , M. Vlajic , P. Erwin , J. Bland-Hawthorn

We model the mass distributions of 40 high surface brightness spiral galaxies inside their optical radii, deriving parameters of mass models by matching the predicted velocities to observed velocity maps. We use constant mass-to-light disk…

Astrophysics · Physics 2009-11-10 Eric I. Barnes , J. A. Sellwood , Arthur Kosowsky

We present decompositions of the rotation curves of three spiral galaxies at redshifts z~0.7 and 1 into contributions by their bulges, disks, and dark halos, respectively. In order to set constraints on the degeneracy of the decompositions…

Astrophysics · Physics 2009-11-10 Burkhard Fuchs , Asmus Boehm , Claus Moellenhoff , Bodo L. Ziegler

We present first results from an on-going survey of the stellar populations of the bulges and inner disks of spirals at various points along the Hubble sequence. In particular, we are investigating the hypotheses that bulges of early-type…

Astrophysics · Physics 2007-05-23 S. C. Trager , J. J. Dalcanton , B. J. Weiner

We study the surface brightness profiles of disc galaxies in the 3.6 micron images from the Spitzer Survey of Stellar Structure in Galaxies (S4G) and K_s-band images from the Near Infrared S0-Sa galaxy Survey (NIRS0S). We particularly…

We present BVI photometry of ten Seyfert 1 galaxies and narrow band H-alpha images for six of these objects as well. The results indicate that the luminosity sample distribution has an amplitude of almost 4 magnitudes with an average of…

Astrophysics · Physics 2009-11-07 N. V. Boris , C. J. Donzelli , M. G. Pastoriza , A. Rodriguez-Ardila , D. L. Ferreiro
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