Search Publications

Subaru Weak Lensing Study of Seven Merging Clusters: Distributions of Mass and Baryons
DOI: 10.1093/pasj/60.2.345 Bibcode: 2008PASJ...60..345O

Umetsu, Keiichi; Okabe, Nobuhiro

We present and compare projected distributions of mass, galaxies, and the intracluster medium (ICM) for a sample of merging clusters of galaxies based on a joint weak-lensing, optical photometric, and X-ray analysis. Our sample comprised seven nearby Abell clusters, for which we had conducted systematic, deep imaging observations with Suprime-Cam …

2008 Publications of the Astronomical Society of Japan
XMM-Newton 168
Suzaku Observations of AWM 7 Cluster of Galaxies: Temperatures, Abundances, and Bulk Motions
DOI: 10.1093/pasj/60.sp1.S333 Bibcode: 2008PASJ...60S.333S

Ishida, Manabu; Sato, Kosuke; Ohashi, Takaya +4 more

We carried out 3 observations of the cluster of galaxies AWM 7, for the central region and 20'-east and 20'-west offset regions, with Suzaku. Temperature and abundance profiles were measured out to 27' simeq 570 h70-1kpc, which corresponded to ∼0.35r180. The temperature of the intra-cluster medium (ICM) slightly de…

2008 Publications of the Astronomical Society of Japan
Suzaku XMM-Newton 53
Suzaku Wide-Band X-Ray Spectroscopy of the Seyfert2 AGN in NGC 4945
DOI: 10.1093/pasj/60.sp1.S251 Bibcode: 2008PASJ...60S.251I

Done, Chris; Isobe, Naoki; Gandhi, Poshak +13 more

Suzaku observed a nearby Seyfert2 galaxy, NGC 4945, which hosts one of the brightest active galactic nuclei above 20keV. Combining data from the two detectors aboard Suzaku, the AGN intrinsic nuclear emission and its reprocessed signals were observed simultaneously. The intrinsic emission is highly obscured with an absorbing column of ∼5×1024…

2008 Publications of the Astronomical Society of Japan
Suzaku XMM-Newton 46
Suzaku Observation of the Metallicity in the Hot Interstellar Medium of the Isolated Elliptical Galaxy NGC 720
DOI: 10.1093/pasj/60.sp1.S307 Bibcode: 2008PASJ...60S.307T

Fukazawa, Yasushi; Anabuki, Naohisa; Matsushita, Kyoko +3 more

The metal abundances in the interstellar medium of the isolated elliptical galaxy NGC 720 were studied with the CCD X-ray Imaging Spectrometer (XIS) aboard the Suzaku satellite. The high detection efficiency along with the excellent spectral resolution of the XIS allowed the K-shell lines of O and Mg to be clearly resolved, and the abundances of O…

2008 Publications of the Astronomical Society of Japan
Suzaku XMM-Newton 23
Suzaku X-Ray Spectroscopy of a Peculiar Hot Star in the Galactic Center Region
DOI: 10.1093/pasj/60.sp1.S173 Bibcode: 2008PASJ...60S.173H

Nagata, Tetsuya; Tsujimoto, Masahiro; Koyama, Katsuji +5 more

We present the results of a Suzaku study of a bright point-like source in the 6.7keV intensity map of the Galactic center region. We detected an intense FeXXV 6.7keV line with an equivalent width of ∼1keV as well as emission lines of highly ionized Ar and Ca from a spectrum obtained by the X-ray Imaging Spectrometer. The overall spectrum is descri…

2008 Publications of the Astronomical Society of Japan
Suzaku XMM-Newton 20
Discovery of a Bright Transient Ultraluminous X-Ray Source, Suzaku J1305-4931 in NGC4945
DOI: 10.1093/pasj/60.sp1.S241 Bibcode: 2008PASJ...60S.241I

Isobe, Naoki; Gandhi, Poshak; Makishima, Kazuo +5 more

An X-ray source, Suzaku J1305-4931, was discovered in the south-west arm of a nearby Seyfert II galaxy, NGC4945, at 0.5-10keV flux of 2.2×10-12erg cm-2 s-1 during a Suzaku observation conducted on 2006 January 15-17. It was undetectable in a shorter observation on 2005 August 22--23, with an upper limit of 1.7×10

2008 Publications of the Astronomical Society of Japan
Suzaku XMM-Newton 15
Implication for Super-Critical Accretion Flow in the Narrow-Line Seyfert 1 Galaxy PKS 0558-504
DOI: 10.1093/pasj/60.3.487 Bibcode: 2008PASJ...60..487H

Kunieda, Hideyo; Haba, Yoshito; Terashima, Yuichi +1 more

We present results from XMM-Newton observations of the narrow-line Seyfert 1 galaxy PKS0558-504. The 2-12keV X-ray spectra can be well-reproduced by a single power law with a photon index of ∼2.2. The extrapolation of this power law continuum into the lower energy band reveals the existence of a strong soft excess component. When we applied a mult…

2008 Publications of the Astronomical Society of Japan
XMM-Newton 9
XMM-Newton Observations of NGC 4051: Temporal Flux and Spectral Variability during Transition to the Faintest Phase in NGC 4051
DOI: 10.1093/pasj/60.6.1257 Bibcode: 2008PASJ...60.1257H

Tsuruta, Sachiko; Liebmann, Andrew C.; Kunieda, Hideyo +2 more

We report on the results from temporal and spectral analyses of NGC 4051 observed with XMM-Newton. The X-ray variabilities in the higher-flux states are well explained by the combination of a variable, direct power law and a temporally stable, absorbed component. In low-flux states, however, spectral variations are mainly due to flux changes of th…

2008 Publications of the Astronomical Society of Japan
XMM-Newton 8
Suzaku Detection of an Intense X-Ray Flare from an A-Type Star, HD161084
DOI: 10.1093/pasj/60.sp1.S49 Bibcode: 2008PASJ...60S..49M

Sugawara, Yasuharu; Maeda, Yoshitomo; Tsujimoto, Masahiro +4 more

We report on a serendipitous detection of an intense X-ray flare from the Tycho reference source on HD161084 during a Suzaku observation of the galactic center region for ∼20ks. The X-ray Imaging Spectrometer recorded a flare from this A1-type dwarf or subgiant star with a flux of ∼1.4 × 10-12 erg s-1 cm-2 (0.5--10…

2008 Publications of the Astronomical Society of Japan
Hipparcos Suzaku XMM-Newton 7
Heavy Element Analysis of X-Ray Faint Elliptical Galaxies
DOI: 10.1093/pasj/60.3.527 Bibcode: 2008PASJ...60..527T

Fukazawa, Yasushi; Tozuka, Miyako

Past ASCA and ROSAT observations could not support the general view that elliptical galaxies are sources of metals in the intracluster medium, since observational results have shown that X-ray faint elliptical galaxies exhibit too low metal abundances of hot interstellar medium (ISM). We investigated the radial profiles of the temperature and abun…

2008 Publications of the Astronomical Society of Japan
XMM-Newton 4