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相关论文: Stellar Population Gradients in Bulges along the H…

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This is the first paper presenting our long-term project aimed at studying the nature of bulges through the analysis of their stellar population gradients. We present deep spectroscopic observations along the minor axis and the data…

天体物理学 · 物理学 2009-11-13 J. Gorgas , P. Jablonka , P. Goudfrooij

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

The radial profiles of the Hb, Mg, and Fe line-strength indices are presented for a sample of eight spiral galaxies with a low surface-brightness stellar disc and a bulge. The correlations between the central values of the line-strength…

宇宙学与河外天体物理 · 物理学 2015-06-04 L. Morelli , E. M. Corsini , A. Pizzella , E. Dalla Bontà , L. Coccato , J. Méndez-Abreu , M. Cesetti

We present first results of a comprehensive survey of deep long-slit spectra along the minor axis of bulges of edge-on spiral galaxies. Our results indicate that stellar populations in bulges are fairly old and encompass a range of…

天体物理学 · 物理学 2009-10-31 P. Goudfrooij , J. Gorgas , P. Jablonka

Photometry and long-slit spectroscopy are presented for 14 S0 and spiral galaxies of the Fornax, Eridanus and Pegasus cluster, and NGC 7582 group. The structural parameters of the galaxies are derived from the R-band images by performing a…

天体物理学 · 物理学 2009-11-13 L. Morelli , E. Pompei , A. Pizzella , J. Méndez-Abreu , E. M. Corsini , L. Coccato , R. P. Saglia , M. Sarzi , F. Bertola

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

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…

天体物理学 · 物理学 2007-05-23 S. C. Trager , J. J. Dalcanton , B. J. Weiner

We have obtained 2D spectral data for a sample of 58 nearby S0 galaxies with the Multi-Pupil Spectrograph of the 6m telescope of the Special Astrophysical Observatory of the Russian Academy of Sciences. The Lick indices H-beta, Mgb, and…

天体物理学 · 物理学 2009-11-13 Olga K. Sil'chenko

We compare the stellar population properties in the central regions of visually classified non-starforming spiral and elliptical galaxies from Galaxy Zoo and SDSS DR7. The galaxies lie in the redshift range $0.04<z<0.1$ and have stellar…

宇宙学与河外天体物理 · 物理学 2015-05-30 Aday R. Robaina , Ben Hoyle , Anna Gallazzi , Raul Jimenez , Arjen van der Wel , Licia Verde

We present photometry and long-slit spectroscopy for 12 S0 and spiral galaxies selected from the Catalogue of Isolated Galaxies. The structural parameters of the sample galaxies are derived from the Sloan Digital Sky Survey i-band images by…

星系天体物理 · 物理学 2016-10-05 L. Morelli , M. Parmiggiani , E. M. Corsini , L. Costantin , E. Dalla Bontà , J. Mèndez-Abreu , A. Pizzella

We present the stellar population and velocity dispersion gradients for a sample of 24 brightest cluster galaxies (BCGs) in the nearby Universe for which we have obtained high quality long-slit spectra at the Gemini telescopes. With the aim…

宇宙学与河外天体物理 · 物理学 2015-06-04 S. I. Loubser , P. Sanchez-Blazquez

This is the second paper of a series aimed to study the stellar kinematics and population properties of bulges in highly-inclined barred galaxies. In this work, we carry out a detailed analysis of the stellar age, metallicity and [Mg/Fe] of…

We have conducted a spectroscopic analysis of the bulges of a sample of 31 spiral galaxies, spanning the Hubble sequence from S0 to Scd type, in order to study the radial distribution of their stellar population properties.

天体物理学 · 物理学 2009-11-07 P. Jablonka , J. Gorgas , P. Goudfrooij

We present a brief summary of our current results on the stellar distribution and population gradients of the resolved stars in the surroundings of ~50 nearby disk galaxies, observed with space- (Hubble & Spitzer) and ground-based…

Radial age gradients hold the cumulative record of the multitude of physical processes driving the build-up of stellar populations and the ensuing star formation (SF) quenching process in galaxy bulges, therefore potentially sensitive…

Key information to understand the formation and evolution of disk galaxies are imprinted in the stellar populations of their bulges. This paper has the purpose to make available new measurements of the stellar population properties of the…

星系天体物理 · 物理学 2015-06-23 L. Morelli , A. Pizzella , E. M. Corsini , E. Dalla Bontà , L. Coccato , J. Méndez-Abreu , M. Parmiggiani

We seek to understand whether the stellar populations of galactic bulges show fingerprints of secular evolution triggered by the presence of the disc. For this purpose we re-analyse the sample of Proctor and Sansom, deriving stellar…

天体物理学 · 物理学 2009-11-13 Daniel Thomas , Roger L. Davies

We analyze the vertical distribution of the resolved stellar populations in six low-mass, edge-on, spiral galaxies observed with the Hubble Space Telescope Advanced Camera for Surveys. In each galaxy we find evidence for an extraplanar…

天体物理学 · 物理学 2008-11-26 Anil C. Seth , Julianne J. Dalcanton , Roelof S. de Jong

We combine the exceptional depth of the Hubble Ultra Deep Field (HUDF) images and the deep GRism ACS Program for Extragalactic Science (GRAPES) grism spectroscopy to explore the stellar populations of 34 bulges belonging to late-type…

天体物理学 · 物理学 2010-10-20 N. P. Hathi , I. Ferreras , A. Pasquali , S. Malhotra , J. E. Rhoads , N. Pirzkal , R. A. Windhorst , C. Xu

For a sample of bright nearby early-type galaxies we have obtained surface photometry in bands ranging from U to K. Since the galaxies have inclinations larger than 50 deg. it is easy to separate bulges and disks. By measuring the colours…

天体物理学 · 物理学 2008-02-03 R. F. Peletier , M. Balcells
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