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相关论文: Photometric Scaling Relations for Bulges of Galaxi…

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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

We investigate bulge and disk scaling relations using a volume-corrected sample of early- to intermediate-type disk galaxies in which, importantly, the biasing flux from additional nuclear components has been modeled and removed. Structural…

天体物理学 · 物理学 2011-02-11 M. Balcells , A. W. Graham , R. F. Peletier

Photometric scaling relations are studied for S0 galaxies and compared with those for spirals. New 2D K_s-band multi-component decompositions are presented for 122 early-type disk galaxies. Combining with our previous decompositions, the…

宇宙学与河外天体物理 · 物理学 2015-05-18 E. Laurikainen , H. Salo , R. Buta , J. H. Knapen , S. Comerón

Bright elliptical galaxies have a markedly different distribution of Hubble types than faint ellipticals; the division occurs near M_B=-20 and bright ellipticals are rounder on average. The Hubble types of galaxies in both groups are…

天体物理学 · 物理学 2009-10-28 Benoit Tremblay , David Merritt

We present deep B- and R-band surface photometry for a sample of 21 galaxies with morphological types between S0 and Sab. We present radial profiles of surface brightness, colour, ellipticity, position angle and deviations of axisymmetry…

天体物理学 · 物理学 2008-11-26 E. Noordermeer , J. M. van der Hulst

We study HST/NICMOS H-band images of bulges of two equal-sized samples of early- (T(RC3) < 4) and late-type spiral (mainly Sbc-Sc) galaxies matched in outer disk axis ratio. We find that bulges of late-type spirals are more elongated than…

天体物理学 · 物理学 2009-11-07 K. Fathi , R. F. Peletier

(Abridged) A variety of formation scenarios was proposed to explain the diversity of properties observed in bulges. Studying their intrinsic shape can help in constraining the dominant mechanism at the epochs of their assembly. The…

天体物理学 · 物理学 2015-05-13 J. Mendez-Abreu , J. A. L. Aguerri , E. M. Corsini , E. Simonneau

We analyzed several basic correlations between structural parameters of galaxies. The data were taken from various samples in different passbands which are available in the literature. We discuss disc scaling relations as well as some…

星系天体物理 · 物理学 2015-06-19 A. V. Mosenkov , N. Ya. Sotnikova , V. P. Reshetnikov

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…

天体物理学 · 物理学 2009-11-10 L. K. Hunt , D. Pierini , C. Giovanardi

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 report the existence of a single plane in the space of global photometric parameters describing elliptical galaxies and the bulges of early type spiral galaxies. The three parameters which define the plane are obtained by fitting the…

天体物理学 · 物理学 2009-10-31 Habib G. Khosroshahi , Yogesh Wadadekar , Ajit Kembhavi , Bahram Mobasher

We present line strengths in the bulges and inner disks of 38 galaxies in the local universe, including several galaxies whose bulges were previously identified as being disk-like in their colors or kinematics, to see if their spectral…

天体物理学 · 物理学 2009-11-11 Bhasker K. Moorthy , Jon A. Holtzman

We summarise some recent results about nearby galactic bulges that are relevant to their formation. We highlight a number of significant advances in our understanding of the surface brightness profiles, stellar populations, and especially…

天体物理学 · 物理学 2007-05-23 Reynier Peletier , Marc Balcells , Jesus Falcon-Barroso , Alister Graham

We present a photometric analysis of a large sample of early-type galaxies in 16 nearby groups, imaged with the Wide-Field Camera on the Isaac Newton Telescope. Using a two-dimensional surface brightness decomposition routine, we fit Sersic…

天体物理学 · 物理学 2009-11-10 H. G. Khosroshahi , S. Raychaudhury , T. J. Ponman , T. A. Miles , D. A. Forbes

We consider the luminosity and environmental dependence of structural parameters of lenticular galaxies in the near-infrared K band. Using a two-dimensional galaxy image decomposition technique, we extract bulge and disk structural…

天体物理学 · 物理学 2014-11-18 Sudhanshu Barway , Yogesh Wadadekar , Ajit K. Kembhavi , Y. D. Mayya

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

We combine deep optical and IR photometry for 326 spiral galaxies from two recent galaxy samples and report that the surface brightness profiles of late-type spirals are best fit by two exponentials. Moreover, the ratio of bulge and disk…

天体物理学 · 物理学 2009-10-28 S. Courteau , R. S. de Jong , A. H. Broeils

We present line-strengths and kinematics from the central regions of 32 galaxies with Hubble types ranging from E to Sbc. Spectral indices, based on the Lick system, are measured in the optical and near infra-red (NIR). The 24 indices…

天体物理学 · 物理学 2008-11-26 R. N. Proctor , A. E. Sansom

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

We investigate the stellar disk properties of a sample of 19 nearby spiral galaxies with low inclination and late Hubble type (Scd or later). We combine our high-resolution HST I-band observations with existing ground-based optical images…

天体物理学 · 物理学 2009-11-07 Torsten Boeker , Rebecca Stanek , Roeland P. van der Marel
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