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相关论文: RX J1548.9+0851, a fossil cluster?

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The most accepted scenario for the origin of fossil groups (FGs) is that they are galaxy associations in which the merging rate was fast and efficient. These systems have assembled half of their mass at early epoch of the Universe,…

We present a detailed X-ray and optical study of a distant fossil system RX J1416.4+2315 (z=0.13), combining Chandra and XMM-Newton observations, optical photometry and spectroscopy. X-ray emitting hot gas imaged by both the Chandra and…

天体物理学 · 物理学 2009-11-11 Habib G. Khosroshahi , Ben J. Maughan , Trevor J. Ponman , Laurence R. Jones

We determine the first fossil group luminosity function based on spectroscopy of the member galaxies. The fossil group RX J1552.2+2013 has 36 confirmed members, it is at a mean redshift of 0.136 and has a velocity dispersion of 623 km/s (or…

天体物理学 · 物理学 2016-08-30 Claudia L. Mendes de Oliveira , Eduardo S. Cypriano , Laerte Sodre

We have discovered a strong lensing fossil group (J0454) at z=0.26, projected near the well-studied cluster MS0451-0305. Using multicolour Subaru/Suprime-Cam and CFHT/Megaprime imaging together with Keck spectroscopy we identify member…

宇宙学与河外天体物理 · 物理学 2011-02-11 Mischa Schirmer , Sherry Suyu , Tim Schrabback , Hendrik Hildebrandt , Aleksi Halkola , Thomas Erben

We use SDSS-DR4 photometric and spectroscopic data out to redshift z~0.1 combined with ROSAT All Sky Survey X-ray data to produce a sample of twenty-five fossil groups (FGs), defined as bound systems dominated by a single, luminous…

It is thought that fossil systems are relics of structure formation in the primitive Universe. They are galaxy aggregations that have assembled their mass at high redshift with few or no subsequent accretion. Observationally these systems…

星系天体物理 · 物理学 2018-01-24 J. A. L. Aguerri , A. Longobardi , S. Zarattini , A. Kundert , E. D'Onghia , L. Dominguez-Palmero

We study the properties of the fossil cluster RX J1416.4+2315 through g' and i'-band imaging and spectroscopy of 25 member galaxies. The system is at a mean redshift of 0.137 and has a velocity dispersion of 584 km s^-1. Superimposed onto…

天体物理学 · 物理学 2008-11-26 Eduardo S. Cypriano , Claudia L. Mendes de Oliveira , Laerte Sodré

Fossil groups are systems with one single central elliptical galaxy and an unusual lack of luminous galaxies in the inner regions. The standard explanation for the formation of these systems suggests that the lack of bright galaxies is due…

宇宙学与河外天体物理 · 物理学 2015-05-13 Claudia L. Mendes de Oliveira , Eduardo S. Cypriano , Renato A. Dupke , Laerte Sodré

We report the discovery of an X-ray luminous galaxy cluster at z=1.26. RXJ0848.9+4452 was selected as an X-ray cluster candidate in the ROSAT Deep Cluster Survey, on the basis of its spatial extent. Deep optical and near-IR imaging have…

We describe the properties of a sample of galaxy groups with very unusual distributions of galaxy luminosities. The most extreme example has an X-ray luminosity similar to that of the Virgo cluster but has a very low richness, with only one…

天体物理学 · 物理学 2009-09-29 L. R. Jones , T. J. Ponman , A. Horton , A. Babul , H. Ebeling , D. J. Burke

We present a photometric and spectroscopic study of stellar populations in the X-ray-luminous cluster of galaxies RXJ0142.0+2131 at z=0.280. This paper analyses the results of high signal-to-noise spectroscopy, as well as g'-, r'-, and…

天体物理学 · 物理学 2008-11-26 Jordi Barr , Roger Davies , Inger Jorgensen , Marcel Bergmann , David Crampton

We report the discovery of an X-ray luminous galaxy cluster at z =1.11. RDCS J0910+5422 was selected as an X-ray cluster candidate in the ROSAT Deep Cluster Survey on the basis of its spatial extent in a Rosat PSPC image. Deep optical and…

天体物理学 · 物理学 2009-11-07 S. A. Stanford , B. P. Holden , P. Rosati , P. R. Eisenhardt , D. Stern , G. Squires , H. Spinrad

Color-magnitude relations have been derived in the clusters RX J0849+4452 and RX J0848+4453 at z~1.26. The color-magnitude relation was determined from Advanced Camera for Surveys imaging in the WFC F775W (i_775) and F850LP (z_850) filters…

We collected multiband imaging and spectroscopy for two fossil groups (RX J1119.7+2126 and 1RXS J235814.4+150524) and one normal group (NGC 6034). We computed photometric redshifts in the central zones of each group, combining previous data…

宇宙学与河外天体物理 · 物理学 2015-06-04 C. Adami , S. Jouvel , L. Guennou , V. LeBrun , F. Durret , B. Clement , N. Clerc , S. Comeron , O. Ilbert , Y. lin , D. Russeil , U. Seemann

This is a report of Chandra, XMM-Newton, HST and ARC observations of an extended X-ray source at z = 0.59. The apparent member galaxies range from spiral to elliptical and are all relatively red (i'-Ks about 3). We interpret this object to…

天体物理学 · 物理学 2009-11-10 M. P. Ulmer , C. Adami , G. Covone , F. Durret , G. B. Lima Neto , K. Sabirli , B. Holden , R. G. Kron , A. K. Romer

We present an X-ray follow-up, based on XMM plus Chandra, of six Fossil Group (FG) candidates identified in our previous work using SDSS and RASS data. Four candidates (out of six) exhibit extended X-ray emission, confirming them as true…

宇宙学与河外天体物理 · 物理学 2015-06-04 F. La Barbera , M. Paolillo , E. De Filippis , R. R. de Carvalho

We present a multi-wavelength study of RX J0848+4456, a cluster of galaxies discovered through X-ray emission in the ROSAT Deep Cluster Survey. Our observations consist of WFPC2 imaging, optical spectra, and X-ray data collected with the…

We report on the discovery of a galaxy cluster at z = 1.490 originally selected as an extended X-ray source in the XMM-Newton Distant Cluster Project. Further observations carried out with the VLT-FORS2 spectrograph allowed the…

We present the results of an extensive spectroscopic survey of RX J0152.7-1357, one of the most massive distant clusters of galaxies known. Multi-object spectroscopy, carried out with FORS1 and FORS2 on the ESO Very Large Telescope (VLT),…

Fossil groups are galaxy structures that probably underwent a nearly complete fusion of all intermediate magnitude galaxies into a single large central dominant galaxy. However, the formation and evolution processes of these structures are…

天体物理学 · 物理学 2009-11-13 C. Adami , D. Russeil , F. Durret
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