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The origin of S0 galaxies is discussed in the framework of early mergers in a Cold Dark Matter cosmology, and in a scenario where S0s are assumed to be former spirals stripped of gas. From an analysis of 127 early-type disk galaxies…

星系天体物理 · 物理学 2009-11-13 E. Laurikainen , H. Salo , R. Buta , J. H. Knapen

We present observations of pseudobulges in S0 and spiral galaxies using imaging data taken with the Spitzer Infra-Red Array Camera. We have used 2-d bulge-disk-bar decomposition to determine structural parameters of 185 S0 galaxies and 31…

星系天体物理 · 物理学 2015-06-24 Kaustubh Vaghmare , Sudhanshu Barway , Smita Mathur , Ajit K. Kembhavi

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 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

We have derived the photometric parameters for the structural components of a sample of fourteen SB0 galaxies by applying a parametric photometric decomposition to their observed $I$-band surface brightness distribution. We find that SB0…

天体物理学 · 物理学 2009-11-10 J. A. L. Aguerri , N. Elias-Rosa , E. M. Corsini , C. Muñoz-Tuñón

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…

天体物理学 · 物理学 2009-11-11 E. Laurikainen , H. Salo , R. Buta , J. Knapen , T. Speltincx , D. Block

It has been recently found that the characteristic photometric parameters of antitruncated discs in S0 galaxies follow tight scaling relations. We investigate if similar scaling relations are satisfied by galaxies of other morphological…

星系天体物理 · 物理学 2015-08-06 M. Carmen Eliche-Moral , Alejandro Borlaff , John E. Beckman , Leonel Gutierrez

About 20% of low-redshift galaxies are late-type spirals with a small or no bulge component. Although they are the simplest disk galaxies in terms of structure and dynamics, the role of the different physical processes driving their…

星系天体物理 · 物理学 2017-05-10 L. Costantin , J. Méndez-Abreu , E. M. Corsini , L. Morelli , J. A. L. Aguerri , E. Dalla Bontà , A. Pizzella

We study the photometric parameters of the bulges of galaxies of different Hubble types including ellipticals, lenticulars, early and late type spirals and early type dwarf galaxies. Analyzing the distributions of various photometric…

天体物理学 · 物理学 2009-11-11 C. D. Ravikumar , Sudhanshu Barway , Ajit Kembhavi , Bahram Mobasher , V. C. Kuriakose

Following from our recent work, we present here a detailed structural analysis of a representative sample of nearby spiral and early-type galaxies taken from the KINGFISH/ SINGS survey. The photometric parameters of bulges are obtained from…

星系天体物理 · 物理学 2021-07-12 Bogdan A. Pastrav

A review of the results of the Near-IR S0 galaxy Survey (NIRS0S) is presented. NIRS0S is a magnitude (mB 12.5 mag) and inclination (< 65o) limited sample of 200 nearby galaxies, mainly S0s. It uses deep Ks -band images, typically reaching a…

宇宙学与河外天体物理 · 物理学 2015-06-03 E. Laurikainen , H. Salo , R. Buta , J. H. Knapen

We have estimated the bulge-to-total ($B/T$) light ratios in the $K_s$-band for a sample of 24 S0, S0/a and Sa galaxies by applying a 2-dimensional multicomponent decomposition method. For the disk an exponential function is used, the…

天体物理学 · 物理学 2009-11-13 Eija Laurikainen , Heikki Salo , Ronald Buta

We measure the scaling relations of the bulges and disks of the EFIGI galaxies in the nearby Universe versus morphology, using bulge and disk decomposition of SDSS gri images with SourceXtractor++. The Kormendy (1977) relation between…

星系天体物理 · 物理学 2024-01-03 Louis Quilley , Valérie de Lapparent

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

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

Galaxy mergers are considered as questionable mechanisms for the evolution of lenticular galaxies (S0's), on the basis that even minor ones induce structural changes that are difficult to reconcile with the strong bulge-disk coupling…

We study a sample of 28 S0 galaxies extracted from the integral-field spectroscopic (IFS) survey CALIFA. We combine an accurate two-dimensional (2D) multi-component photometric decomposition with the IFS kinematic properties of their bulges…

Type-III S0 galaxies present tight scaling relations between their surface brightness photometric and structural parameters. Several evolutionary models have been proposed for the formation of Type-III S0 galaxies but the observations of…

Lenticular galaxies (S0s) represent the majority of early-type galaxies in the local Universe, but their formation channels are still poorly understood. While galaxy mergers are obvious pathways to suppress star formation and increase bulge…

From a diameter-limited sample of 86 `face-on' spiral galaxies, the bulge-to-disk size and luminosity ratios, and other quantitative measurements for the prominence of the bulge are derived. The bulge and disk parameters have been estimated…

天体物理学 · 物理学 2012-04-26 Alister W. Graham
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