中文
相关论文

相关论文: Soft band X/K luminosity ratios for gas-poor early…

200 篇论文

We study X-ray to K-band luminosity ratios (L_X/L_K) of late-type galaxies in the 0.3-0.7 keV energy range. From the Chandra archive, we selected nine spiral and three irregular galaxies with point source detection sensitivity better than 5…

高能天体物理现象 · 物理学 2015-05-20 Akos Bogdan , Marat Gilfanov

We explore the nature of unresolved X-ray emission in a broad sample of galaxies of all morphological types based on archival Chandra data. After removing bright compact sources, we study L_X/L_K luminosity ratios of unresolved emission,…

高能天体物理现象 · 物理学 2015-05-28 Akos Bogdan , Marat Gilfanov

We have selected a sample of 30 normal (non-cD) early type galaxies, for all of which optical spectroscopy is available, and which have been observed with Chandra to a depth such to insure the detection of bright low-mass X-ray binaries…

高能天体物理现象 · 物理学 2015-05-20 Bram Boroson , Dong-Woo Kim , Giuseppina Fabbiano

We study populations of soft and super-soft X-ray sources in nearby galaxies of various morphological types with the special emphasis on characterizing populations of stable nuclear burning accreting WDs. Analysing the content of Chandra…

高能天体物理现象 · 物理学 2021-02-17 I. Galiullin , M. Gilfanov

We investigated the X-ray spectral properties of a collection of low-mass X-ray binaries (LMXBs) within a sample of 15 nearby early-type galaxies observed with Chandra. We find that the spectrum of the sum of the sources in a given galaxy…

天体物理学 · 物理学 2009-11-07 Jimmy A. Irwin , Alex E. Athey , Joel N. Bregman

We have identified 127 discrete sources in a Chandra observation of M83, with a detection limit of ~ 3 x 10^{36} erg/s in the 0.3-8.0 keV band. We discuss the individual properties of about 20 bright sources with L_x >~ 10^{38} erg/s, and…

天体物理学 · 物理学 2009-11-10 Roberto Soria , Kinwah Wu

The results of a 0.4-10.0 keV ASCA spectral analysis of a sample of low-luminosity AGN (LLAGN; M51, NGC 3147, NGC 4258), low-ionization nuclear emission line regions (LINERs; NGC 3079, NGC 3310, NGC 3998, NGC 4579, NGC 4594) and starburst…

天体物理学 · 物理学 2009-10-30 A. Ptak , P. Serlemitsos , T. Yaqoob , R. Mushotzky

A Chandra ACIS-S imaging observation of the nearby galaxy M81 (NGC 3031) reveals 9 luminous soft X-ray sources. The local environments, X-ray spectral properties, and X-ray light curves of the sources are presented and discussed in the…

天体物理学 · 物理学 2009-11-07 Douglas Swartz , Kajal Ghosh , Valery Suleimanov , Allyn Tennant , Kinwah Wu

We study a sample of 69 X-ray detected Early Type Galaxies (ETGs), selected from the Chandra COSMOS survey, to explore the relation between the X-ray luminosity of hot gaseous halos (L_X, gas) and the integrated stellar luminosity (L_K) of…

星系天体物理 · 物理学 2015-06-19 F. Civano , G. Fabbiano , S. Pellegrini , D-W. Kim , A. Paggi , R. Feder , M. Elvis

We investigate the serendipitous X-ray source population revealed in XMM-Newton observations targeted in the Galactic Plane within the region 315<l<45 and |b|<2.5 deg. Our study focuses on a sample of 2204 X-ray sources at intermediate to…

星系天体物理 · 物理学 2015-05-20 R. S. Warwick , D. Perez-Ramirez , K. Byckling

We have analyzed Chandra observations of 18 low-luminosity early-type galaxies with L_B < 3 x 10e10 Lo. Thermal emission from hot gas with temperatures between 0.2 and 0.8 keV comprises 5-70% of the total 0.5-2.0 keV emission from these…

天体物理学 · 物理学 2008-11-26 Laurence P. David , Christine Jones , William Forman , Iris Monica Vargas , Paul Nulsen

Nuclear hard X-ray luminosities (Lx,nuc) for a sample of 112 early type galaxies within a distance of 67 Mpc are used to investigate their relationship with the central galactic black hole mass Mbh, the inner galactic structure (using the…

星系天体物理 · 物理学 2015-05-19 S. Pellegrini

A recent re-analysis of Einstein data, and new ROSAT observations, have revealed the presence of at least two components in the X-ray spectra of X-ray faint early-type galaxies: a relatively hard component (kT>1.5 keV), and a very soft…

天体物理学 · 物理学 2010-12-13 S. Pellegrini , G. Fabbiano

We analyze archival ROSAT HRI, ROSAT PSPC, and ASCA data of the X-ray faint early-type galaxy NGC4697. The joint ROSAT PSPC + ASCA spectrum is fit by a two-component thermal model, a MEKAL model with kT_{MEKAL}=0.26^{+0.04}_{-0.03} keV with…

天体物理学 · 物理学 2009-10-31 Jimmy A. Irwin , Craig L. Sarazin , Joel N. Bregman

This paper uses the 1st XMM Serendipitous Source Catalog compiled by the XMM Science Center to identify low-z X-ray selected normal galaxy candidates. Our sample covers a total area of ~6deg^2 to the 0.5-2keV limit 1e-15cgs. A total of 23…

天体物理学 · 物理学 2009-11-11 A Georgakakis , V. Chavushyan , M. Plionis , I. Georgantopoulos , E. Koulouridis , I. Leonidaki , A. Mercado

We present a sample of hard X-ray selected candidate black holes (BHs) in 19 dwarf galaxies. BH candidates are identified by cross-matching a parent sample of ~44,000 local dwarf galaxies (M_stellar < 3 x 10^9 Msun, z<0.055) with the…

星系天体物理 · 物理学 2015-05-27 Sean Lemons , Amy Reines , Richard Plotkin , Elena Gallo , Jenny Greene

(abridged) We present an analysis of Chandra X-ray observations of a sample of eight dwarf starburst galaxies (I Zw 18, VII Zw 403, NGC 1569, NGC 3077, NGC 4214, NGC 4449, NGC 5253, and He 2-10). Extended, diffuse X-ray emission is detected…

天体物理学 · 物理学 2009-11-10 Juergen Ott , Fabian Walter , Elias Brinks

We present results of morphological and spectroscopic study of hot gas in some early-type galaxies based on the analysis of high resolution X-ray images acquired from the archive of Chandra space mission. Distribution of the hot gas in…

宇宙学与河外天体物理 · 物理学 2009-03-19 N. D. Vagshette , M. K. Patil , S. K. Pandey , Ajit Kembhavi

We present a study of the X-ray properties of a sample of six nearby late-type spiral galaxies based on XMM-Newton observations. Since our primary focus is on the linkage between X-ray emission and star formation in extended, extranuclear…

星系天体物理 · 物理学 2015-05-13 R. A. Owen , R. S. Warwick

We have carried out an in-depth study of low-mass X-ray binaries (LMXBs) detected in the nearby lenticular galaxy NGC 3115, using the Megasecond Chandra X-Ray Visionary Project observation (total exposure time 1.1 Ms). In total we found 136…

‹ 上一页 1 2 3 10 下一页 ›