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相关论文: Multicomponent Decompositions for a Sample of S0 g…

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Using high-quality optical images from the Carnegie-Irvine Galaxy Survey, we perform multi-component decompositions of S0 galaxies to derive accurate structural parameters to constrain their physical origin. Many S0s do not host prominent…

星系天体物理 · 物理学 2018-07-31 Hua Gao , Luis C. Ho , Aaron J. Barth , Zhao-Yu Li

We use the Spitzer Survey of Stellar Structure in Galaxies (S$^{4}$G) 3.6 $\mu$m imaging to study the properties (length and strength) and fraction of bars at $z=0$. We use the maximum of tangential-to-radial force ratio in the bar region…

星系天体物理 · 物理学 2016-07-26 Simón Díaz-García , Heikki Salo , Eija Laurikainen , Martín Herrera-Endoqui

We present a sample of edge-on spiral galaxies both of early and late types.The sample consists of 175 galaxies in the Ks-filter, 169 galaxies in the H-filter and 165 galaxies in the J-filter. Bulge and disc decompositions of each galaxy…

宇宙学与河外天体物理 · 物理学 2010-12-16 N. Ya. Sotnikova , V. P. Reshetnikov , A. V. Mosenkov

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

A panchromatic investigation of morphology for the early-type spiral galaxy M81 is presented in this paper. We perform bulge-disk decomposition in M81 images at a total of 20 wavebands from FUV to NIR obtained with GALEX, Swift, SDSS, WIYN,…

星系天体物理 · 物理学 2023-07-26 Jun-Yu Gong , Ye-Wei Mao , Hua Gao , Si-Yue Yu

Using data from the Near-Infrared S0 Survey (NIRS0S) of nearby, early-type galaxies, we examine the distribution of bar strengths in S0 galaxies as compared to S0/a and Sa galaxies, and as compared to previously published bar strength data…

星系天体物理 · 物理学 2015-05-19 R. Buta , E. Laurikainen , H. Salo , J. Knapen

A sample of edge-on spiral galaxies aimed at a study of the main structural and photometric parameters of edge-on galaxies both of early and late types is presented. The data were taken from the 2MASS in the J, H and K_s filters. The sample…

宇宙学与河外天体物理 · 物理学 2015-05-14 A. V. Mosenkov , N. Ya. Sotnikova , V. P. Reshetnikov

The structural parameters of a magnitude-limited sample of 148 unbarred S0-Sb galaxies were derived to study the correlations between bulge and disk parameters as well as the probability distribution function (PDF) of the intrinsic…

天体物理学 · 物理学 2008-02-04 J. Méndez-Abreu , J. A. L. Aguerri , E. M. Corsini , E. Simonneau

We have modelled the light distribution in 10095 galaxies from the Millennium Galaxy Catalogue (MGC), providing publically available structural catalogues for a large, representative sample of galaxies in the local Universe. Three different…

From a purely photometric perspective galaxies are generally decomposed into a bulge+disc system, with bulges being dispersion-dominated and discs rotationally-supported. However, recent observations have demonstrated that such a framework…

We investigate the morphology and structural properties of 246 massive compact quiescent galaxies (MCGs; $\log M_{\star} \sim 10$-$11$, $\sigma_{\mathrm{e}} \sim 150$-$350\,$km\,s$^{-1}$, $R_{\mathrm{e}} \sim 0.7$-$2.5\,$kpc) at $z \sim 0$,…

We present near-infrared (NIR) surface photometry of a sample of 14 early-type spirals with observed rotation curves. In this first paper, we report the results of two-dimensional parametric and non-parametric decompositions to separate the…

天体物理学 · 物理学 2009-10-30 Giovanni Moriondo , Carlo Giovanardi , Leslie K. Hunt

Different processes have been proposed to explain the formation of S0s, including mergers, disc instabilities and quenched spirals. These processes are expected to dominate in different environments, and thus leave characteristic footprints…

Recent observations and simulations have shown that a buckled bar in the face-on view can be considered as a combination of a long flat bar and a short round barlens (corresponding to the boxy/peanut bulge in the edge-on view). However, the…

星系天体物理 · 物理学 2025-10-15 Xinyang Li , Zhao-Yu Li , Yang A. Li , Ming-Yang Zhuang , Xiaojie Liao

We present here a thorough photometric analysis of double-barred galaxies, consisting of i) two-dimensional photometric decompositions including a bulge, inner bar, outer bar, and (truncated) disc; and ii) three-dimensional statistical…

星系天体物理 · 物理学 2019-01-23 A. de Lorenzo-Cáceres , J. Méndez-Abreu , B. Thorne , L. Costantin

Observations reveal a strong structural coupling between bulge and disc in S0 galaxies, which seems difficult to explain if they have formed from supposedly catastrophic events such as major mergers. We face this question by quantifying the…

星系天体物理 · 物理学 2014-12-24 M. Querejeta , M. C. Eliche-Moral , T. Tapia , A. Borlaff , C. Rodríguez-Pérez , J. Zamorano , J. Gallego

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…

星系天体物理 · 物理学 2016-07-20 Keunho Kim , Sree Oh , Hyunjin Jeong , Alfonso Aragon-Salamanca , Rory Smith , Sukyoung K. Yi

We present a study of low surface brightness galaxies (LSBGs) selected by fitting the images for all the galaxies in $\alpha$.40 SDSS DR7 sample with two kinds of single-component models and two kinds of two-component models (disk+bulge):…

星系天体物理 · 物理学 2023-12-14 Bing-qing Zhang , Hong Wu , Wei Du , Pin-song Zhao , Min He , Feng-jie Lei

The structural parameters of bulges, disks and bars of a sample of nearly 1000 nearby galaxies are being determined through sophisticated image decomposition in the g, r and i bands. The sample is carefully drawn from the Sloan Digital Sky…

天体物理学 · 物理学 2009-11-13 Dimitri Gadotti , Guinevere Kauffmann

We present a detailed morphological, photometric, and kinematic analysis of two barred S0 galaxies with large, luminous inner disks inside their bars. We show that these structures, in addition to being geometrically disk-like, have…

天体物理学 · 物理学 2009-11-10 Peter Erwin , Juan Carlos Vega Beltran , Alister W. Graham , John E. Beckman