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Related papers: X-Ray Properties of Early Type Galaxies as Observe…

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We present an analysis of 39 X-ray luminous early-type galaxies observed with the ROSAT PSPC. Using multi-component spectral and spatial fits to these data we have measured halo abundance, temperature, luminosity and surface brightness…

Astrophysics · Physics 2009-11-07 Ewan O'Sullivan , Trevor J. Ponman , Ross S. Collins

(Abridged) I present a comprehensive and uniform analysis of 25 {\it ASCA} observations from 23 Narrow-line Seyfert 1 galaxies. The time series analysis is presented in this paper, Part 1, and the spectral analysis and correlations are…

Astrophysics · Physics 2009-10-31 Karen M. Leighly

(Abridged) I present a comprehensive and uniform analysis of 25 {\it ASCA} observations from 23 Narrow-line Seyfert 1 galaxies. The spectral analysis and correlations are presented in this paper, Part 2; the reduction and time series…

Astrophysics · Physics 2008-11-26 Karen M. Leighly

Hubble Space Telescope observations revealed that the central surface brightness profiles of early type galaxies can be divided into two types: "core" profiles and featureless power law profiles. On the basis of this and previous results,…

Astrophysics · Physics 2007-05-23 S. Pellegrini

A sample of nearly 9000 early-type galaxies, in the redshift range 0.01 < z < 0.3, was selected from the Sloan Digital Sky Survey using morphological and spectral criteria. This paper describes how the sample was selected, presents examples…

We present the first in a series of papers describing the X-ray properties of a sample of 18 Seyfert 1 galaxies, using data obtained by \asca. The imaging data reveal a number of serendipitous hard X-ray sources in some source fields, but…

Astrophysics · Physics 2008-11-26 K. Nandra , I. M. George , R. F. Mushotzky , T. J. Turner , T. Yaqoob

To test the cooling flow model of early-type galaxies, we obtained a complete magnitude-limited sample of 34 early-type galaxies, observed with the PSPC and HRI on ROSAT. The X-ray to optical distribution of galaxies implies a lower…

Astrophysics · Physics 2009-10-30 Beth A. Brown , Joel N. Bregman

We investigate the evolution over the last 6.3 Gyr of cosmic time (i.e., since z ~ 0.7) of the average X-ray properties of early-type galaxies within the Extended Chandra Deep Field-South (E-CDF-S). Our early-type galaxy sample includes 539…

Statistical properties of X-ray luminosity and temperature are studied for 52 early-type galaxies based on the ROSAT PSPC data. All of the X-ray luminous galaxies show largely extended emission with a radius of a few times of 10$r_e$, while…

Astrophysics · Physics 2009-10-31 Kyoko Matsushita

Optically-similar early-type galaxies are observed to have a large and poorly understood range in the amount of hot, X-ray-emitting gas they contain.To investigate the origin of this diversity, we studied the hot gas properties of all 42…

Astrophysics of Galaxies · Physics 2015-04-07 Yuanyuan Su , Jimmy A. Irwin , Raymond E. White , Michael C. Cooper

We identify a spectroscopic sequence of galaxies, analogous to the Hubble sequence of morphological types, based on the Automatic Spectroscopic K-means (ASK) classification. Considering galaxy spectra as multidimensional vectors, the…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-27 Yago Ascasibar , Jorge Sanchez-Almeida

Early-type dwarf galaxies, once believed to be simple systems, have recently been shown to exhibit an intriguing diversity in structure and stellar content. To analyze this further, we started the SMAKCED project, and obtained deep H-band…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-03 J. Janz , E. Laurikainen , T. Lisker , H. Salo , R. F. Peletier , S. -M. Niemi , M. den Brok , E. Toloba , J. Falcón-Barroso , A. Boselli , G. Hensler

The ASCA satellite made 107 pointing observations on a 5 x 5 deg^2 region around the center of our Milky Way Galaxy (the Galactic Center) from 1993 to 1999. In the X-ray images of the 0.7--3 keV or 3--10 keV bands, we found 52 point sources…

One hundred and six galaxy clusters have been studied in detail using X-ray data and important global physical properties have been determined. Correlations between these properties are studied with respect to the description of clusters as…

Astrophysics · Physics 2007-05-23 Thomas H. Reiprich , Hans Boehringer

This paper reports on a near-infrared survey of early-type galaxies designed to provide information on bar strengths, bulges, disks, and bar parameters in a statistically well-defined sample of S0-Sa galaxies. Early-type galaxies have the…

Astrophysics · Physics 2008-11-26 R. Buta , E. Laurikainen , H. Salo , D. L. Block , J. H. Knapen

This paper presents a comprehensive study of the X-ray properties of low-ionization nuclear emission-line regions (LINERs) and low-luminosity Seyfert galaxies based on observations obtained with ASCA. We analyzed data of 53 observations of…

Astrophysics · Physics 2009-11-07 Yuichi Terashima , Naoko Iyomoto , Luis C. Ho , Andrew F. Ptak

We have found the stellar populations of early-type galaxies are homogeneous with no significant difference in color or Mg2 index, despite the dichotomy between X-ray extended early-type galaxies and X-ray compact ones. Since the X-ray…

Astrophysics · Physics 2009-10-31 T. Kodama , K. Matsushita

The colors and chemical abundances of early-type galaxies at redshifts z<0.3 are studied using a sample of nearly 9000 galaxies, selected from the Sloan Digital Sky Survey using morphological and spectral criteria. In this sample, redder…

The results of photometric decomposition of surface brightness distributions in 85 early-type unbarred galaxies are presented. The SDSS r-images are analysed. Double-tiered exponential disks are found in all galaxies which are studied; the…

Cosmology and Nongalactic Astrophysics · Physics 2010-12-08 Marina A. Ilyina , Olga K. Sil'chenko

We combine Sloan Digital Sky Survey spectra of 22,000 luminous, red, bulge-dominated galaxies to get high S/N average spectra in the rest-frame optical and ultraviolet (2600A to 7000A). The average spectra of these massive, quiescent…

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