Search Publications

The XMM cluster outskirts project (X‑ COP )
DOI: 10.1002/asna.201713345 Bibcode: 2017AN....338..293E

Pointecouteau, E.; Paltani, S.; Molendi, S. +3 more

Galaxy clusters are thought to grow hierarchically through the continuous merging and accretion of smaller structures across cosmic time. In the local Universe, these phenomena are still active in the outer regions of massive clusters ($R>R_{500}$), where the matter distribution is expected to become clumpy and asymmetric because of the presenc…

2017 Astronomische Nachrichten
Planck Suzaku XMM-Newton 95
Accretion disk winds in active galactic nuclei: X-ray observations, models, and feedback
DOI: 10.1002/asna.201612322 Bibcode: 2016AN....337..410T

Tombesi, F.

Powerful winds driven by active galactic nuclei (AGN) are often invoked to play a fundamental role in the evolution of both supermassive black holes (SMBHs) and their host galaxies, quenching star formation and explaining the tight SMBH-galaxy relations. A strong support of this ``quasar mode'' feedback came from the recent X-ray observation of a …

2016 Astronomische Nachrichten
Suzaku 13
The peculiar megamaser AGN NGC 1194: Comparison with the warped disk candidates NGC 1068 and NGC 4258
DOI: 10.1002/asna.201512272 Bibcode: 2016AN....337...96F

Vasylenko, A.; Fedorova , E.; Hnatyk, B. I. +1 more

We analyze the X-ray properties of the Compton-thick Seyfert 1.9 radio quiet AGN in NGC 1194 using INTEGRAL (ISGRI), XMM-Newton (EPIC), Swift (BAT and XRT), and Suzaku (XIS) observations. There is a set of Fe-K lines in the NGC 1194 spectrum with complex relativistic profiles that can be considered as a sign of either a warped Bardeen-Petterson ac…

2016 Astronomische Nachrichten
INTEGRAL Suzaku XMM-Newton 5
Broadband short term X-ray variability of the quasar PDS 456
DOI: 10.1002/asna.201612336 Bibcode: 2016AN....337..495M

Tombesi, F.; Reeves, J. N.; Braito, V. +4 more

We present a detailed analysis of a recent 500 ks net exposure Suzaku observation, carried out in 2013, of the nearby (z=0.184) luminous (L_bol∼1047 erg s-1) quasar PDS 456 in which the X-ray flux was unusually low. The short term X-ray spectral variability has been interpreted in terms of variable absorption and/or intrinsic…

2016 Astronomische Nachrichten
Suzaku XMM-Newton 4
A new characterization of the Compton process in the ULX spectra
DOI: 10.1002/asna.201612333 Bibcode: 2016AN....337..479K

Makishima, K.; Kobayashi, S.; Nakazawa, K.

Attempts were made to construct a unified description of the spectra of ULX (Ultra Luminous X-ray source) objects, including their power-law (PL) state and disk-like state. Among spectral models proposed to explain either state, the present work adopts the one which combines multi-color disk (MCD) emission and its thermal Comptonization (THC). Thi…

2016 Astronomische Nachrichten
Suzaku XMM-Newton 3
Broadband X-ray study of the galactic black hole binary 4U 1630-47 with Suzaku
DOI: 10.1002/asna.201612331 Bibcode: 2016AN....337..467H

Done, C.; Hori, T.; Shidatsu, M. +4 more

We present the results from our Suzaku observations of the Galactic black hole binary 4U 1630-47. 4U 1630-47 was observed in the very high state (VHS) during the 2012 September-October outburst. The inner disk appears slightly truncated by comparison with a previous high/soft state (HSS) of this source, even by taking into account energetic coupli…

2016 Astronomische Nachrichten
Suzaku 1
Variability of the X-ray broad iron spectral features in active galactic nuclei and black-hole binaries
DOI: 10.1002/asna.201612338 Bibcode: 2016AN....337..507M

Tsujimoto, M.; Ebisawa, K.; Inoue, H. +1 more

The ``broad iron spectral features'' are often seen in X-ray spectra of active galactic nuclei (AGN) and black-hole binaries (BHB). These features may be explained either by the ``relativistic disc reflection'' scenario or the ``partial covering'' scenario: It is hardly possible to determine which model is valid from time-averaged spectral analysi…

2016 Astronomische Nachrichten
Suzaku XMM-Newton 1
Merger shocks in Abell 3667 and the Cygnus A cluster
DOI: 10.1002/asna.201211854 Bibcode: 2013AN....334..346S

Finoguenov, A.; Wik, D. R.; Sarazin, C. L.

We present new XMM-Newton observations of the northwest (NW) radio relic region in the cluster Abell 3667. We detect a jump in the X-ray surface brightness and X-ray temperature at the sharp outer edge of the radio relic which indicate that this is the location of a merger shock with a Mach number of about 2. Comparing the radio emission to the sh…

2013 Astronomische Nachrichten
Suzaku XMM-Newton 23
Bulk motion measurements in clusters of galaxies with ATHENA-like missions
DOI: 10.1002/asna.201211849 Bibcode: 2013AN....334..321N

Nevalainen, J.

The hierarchical formation of clusters of galaxies by accretion of material releases gravitational energy which dissipates into the intracluster gas. The process heats the material and generates gas turbulence and bulk motions and thus kinetic pressure. Mapping the velocity fields of the moving subunits would enable a new diagnostics tool for clus…

2013 Astronomische Nachrichten
Suzaku 5
X-ray measurement of the elemental abundances at the outskirts of the Perseus cluster with Suzaku
DOI: 10.1002/asna.201211872 Bibcode: 2013AN....334..426U

Hayashida, K.; Tsunemi, H.; Ueda, S. +1 more

We report on the abundance of metals (Mg and Fe) in the intracluster medium (ICM) at the outskirts (0.2 r200-0.8 r200) of the Perseus cluster. The X-ray spectra were obtained in the Suzaku/XIS mapping observations of this region. We employ single temperature models to fit all the X-ray spectra. The ICM temperature smoothly de…

2013 Astronomische Nachrichten
Suzaku 4