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Related papers: Cavities, shocks and a cold front around 3C 320

200 papers

We present deep emission-line imaging taken with the SOAR Optical Imaging Camera of the brightest cluster galaxy (BCG) in the nearby (z=0.035) X-ray cluster 2A0335+096. We analyze long-slit optical spectroscopy, archival VLA, Chandra X-ray,…

Astrophysics · Physics 2009-06-23 Megan Donahue , Ming Sun , Christopher P. O'Dea , G. Mark Voit , Kenneth W. Cavagnolo

We present the analysis of 30 ksec of Chandra observations of the galaxy cluster Abell 1835. Overall, the X-ray image shows a relaxed morphology, although we detect substructure in in the inner 30 kpc radius. Spectral analysis shows a steep…

Astrophysics · Physics 2009-09-17 R. W. Schmidt , S. W. Allen , A. C. Fabian

We present the results of 20 ksec Chandra observations for each of 5 radio galaxies in the redshift range 2.0 < z < 2.6. For 4 of the 5 targets we detect unresolved X-ray components coincident with the radio nuclei. From spectral analysis…

A number of merging galaxy clusters shows the presence of shocks and cold fronts, i.e. sharp discontinuities in surface brightness and temperature. The observation of these features requires an X-ray telescope with high spatial resolution…

High Energy Astrophysical Phenomena · Physics 2018-04-17 A. Botteon , F. Gastaldello , G. Brunetti

We present results from a Chandra X-ray Observatory study of the field X-ray source populations in 4 different observations: two high-redshift (z~0.5) clusters of galaxies 3C295 and RXJ003033.2+261819; and two non-cluster fields with…

We present the first X-ray dedicated study of the galaxy cluster A795 and of the Fanaroff-Riley Type 0 hosted in its brightest cluster galaxy. Using an archival 30 ks \textit{Chandra} observation we study the dynamical state and cooling…

Astrophysics of Galaxies · Physics 2021-03-31 Francesco Ubertosi , Myriam Gitti , Eleonora Torresi , Fabrizio Brighenti , Paola Grandi

We present results from a 140 ks Chandra/ACIS-S observation of the hot gas around the canonical FR I radio galaxy 3C 449. An earlier, shorter 30 ks Chandra observation of the group gas showed an unusual entropy distribution and a surface…

Gemini Multi Object Spectrograph medium-resolution spectra and photometric data of 39 objects in the field of the radio galaxy 3C 17 are presented. Based on the new data, a previously uncataloged cluster of galaxies is identified at a mean…

We present a Chandra observation of the central (r< 200kpc) region of the cluster of galaxies 2A 0335+096, rich in interesting phenomena. On large scales (r> 40kpc), the X-ray surface brightness is symmetric and slightly elliptical. The…

Astrophysics · Physics 2009-11-07 Pasquale Mazzotta , Alastair Edge , Maxim Markevitch

We present results based on the systematic analysis of high resolution 95 ks Chandra observations of the strong cool core cluster Abell 2390 at the redshift of z= 0.228 that hosts an energetic radio AGN. This analysis has enabled us to…

Cosmology and Nongalactic Astrophysics · Physics 2024-06-24 S. S. Sonkamble , N. D. Vagshette , P. K. Pawar , M. K. Patil

We report the Chandra discovery of an X-ray cluster at redshift z = 1.063 associated with the Compact Steep Spectrum radio loud quasar 3C 186 (Q0740+380). Diffuse X-ray emission is detected out to ~120 kpc from the quasar and contains…

We present a detailed analysis of jet activity in the radio galaxy 3C348 at the center of the galaxy cluster Hercules A. We use archival Chandra data to investigate the jet-driven shock front, the radio-faint X-ray cavities, the eastern…

High Energy Astrophysical Phenomena · Physics 2025-01-15 F. Ubertosi , Y. Gong , P. Nulsen , J. P. Leahy , M. Gitti , B. R. McNamara , M. Gaspari , M. Singha , C. O'Dea , S. Baum

We present results from {\em Chandra}/ACIS-S, {\em Spitzer}, {\em XMM-Newton}, {\em HST}, and VLA observations of the radio hot spots, extended environment, and nucleus of the nearby ($z$=0.0597) FR II radio galaxy 3C 33. This is a…

We present the results of a Chandra observation of the cooling core cluster Abell 2063. Spectral analysis shows that there is cool gas (2 keV) associated with the cluster core, which is more than a factor of 2 cooler than the outer cluster…

Astrophysics · Physics 2008-11-26 Kalin N. Kanov , Craig L. Sarazin , Amalia K. Hicks

We present observations of four z>= SDSS quasars at 350 micron with the SHARC-II bolometer camera on the Caltech Submillimeter Observatory. These are among the deepest observations that have been made by SHARC-II at 350 micron, and three…

We present a 100 ks Chandra observation studying the extended X-ray emission around the powerful z=1.04 quasar PKS1229-021. The diffuse cluster X-ray emission can be traced out to ~15 arcsec (~120 kpc) radius and there is a drop in the…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-03 H. R. Russell , A. C. Fabian , G. B. Taylor , J. S. Sanders , K. M. Blundell , C. S. Crawford , R. M. Johnstone , E. Belsole

We present results from an analysis of two Chandra observations of the rich, nearby galaxy cluster Abell 2199. We find evidence (having corrected for projection effects) for radial gradients in temperature and metallicity in the X-ray…

Astrophysics · Physics 2009-09-17 R. M. Johnstone , S. W. Allen , A. C. Fabian , J. S. Sanders

We present the spectral analysis of a 200~ks observation of the broad-line radio galaxy 3C~120 performed with the high energy transmission grating (HETG) spectrometer on board the \emph{Chandra} X-ray Observatory. We find (i) a neutral…

High Energy Astrophysical Phenomena · Physics 2017-03-29 F. Tombesi , R. F. Mushotzky , C. S. Reynolds , T. Kallman , J. N. Reeves , V. Braito , Y. Ueda , M. A. Leutenegger , B. J. Williams , L. Stawarz , M. Cappi

Using a 90 ks Chandra ACIS-S observation in the 0.3--7 keV band, along with complementary Low-Frequency Array and Karl G.~Jansky Very Large Array data in the 120--168 MHz and 1--2 GHz ranges, we study the diffuse emission around the nearby…

High Energy Astrophysical Phenomena · Physics 2025-08-19 Q. Daniel Wang , Juergen Ott

We present optical photometric and polarimetric observations of stars towards NGC 1931 with the aim to derive the cluster parameters such as distance, reddening, age and luminosity/mass function as well as to understand the dust properties…

Solar and Stellar Astrophysics · Physics 2015-06-12 A. K. Pandey , C. Eswaraiah , Saurabh Sharma , M. R. Samal , N. Chauhan , W. P. Chen , J. Jose , D. K. Ojha , Ram Kesh Yadav , H. C. Chandola