Search Publications

The Origin of an Extended X-Ray Emission Apparently Associated with the Globular Cluster 47 Tucanae
DOI: 10.1093/pasj/61.5.1107 Bibcode: 2009PASJ...61.1107Y

Makishima, Kazuo; Nakazawa, Kazuhiro; Yuasa, Takayuki

Using the Suzaku X-ray Imaging Spectrometer, we performed a 130 ks observation of an extended X-ray emission, which was shown by ROSAT and Chandra observations to apparently associate with the globular cluster 47 Tucanae. The obtained 0.5-6 keV spectrum was successfully fitted with a redshifted thin thermal plasma emission model whose temperature …

2009 Publications of the Astronomical Society of Japan
Suzaku 8
Another Abundance Inhomogeneity in the South East Limb of the Cygnus Loop
DOI: 10.1093/pasj/61.sp1.S147 Bibcode: 2009PASJ...61S.147T

Katsuda, Satoru; Uchida, Hiroyuki; Mori, Koji +2 more

We observed the south east (SE) limb of the Cygnus Loop with Suzaku. Our spatially-resolved spectroscopic study shows that a one-kTe non-equilibrium ionization model represents our spectra fairly well. We find that the metal abundances obtained are all depleted relative to the solar values with a positional dependence along the radial d…

2009 Publications of the Astronomical Society of Japan
Suzaku 8
Discoveries of 3 K-Shell Lines of Iron and a Coherent Pulsation of 593s from SAX J1748.2-2808
DOI: 10.1093/pasj/61.sp1.S93 Bibcode: 2009PASJ...61S..93N

Koyama, Katsuji; Matsumoto, Hironori; Nobukawa, Masayoshi +1 more

SAX J1748.2-2808 is a unique X-ray object with a flat spectrum and strong emission lines at 6.4--7.0keV. The Suzaku satellite resolved the emission lines into 3 K-shell lines from neutral and highly ionized irons. A clear coherent pulsation with a period of 593s was found from the Suzaku and XMM-Newton archives. These facts favor that SAX J1748.2-…

2009 Publications of the Astronomical Society of Japan
Suzaku XMM-Newton 8
Broad-Band Spectrum of the Black Hole Candidate IGR J17497-2821 Studied with Suzaku
DOI: 10.1093/pasj/61.sp1.S107 Bibcode: 2009PASJ...61S.107P

Dotani, Tadayasu; Yamaoka, Kazutaka; Kokubun, Motohide +9 more

The broad-band 1--300keV Suzaku spectrum of IGR J17497-2821, the X-ray transient discovered by INTEGRAL in 2006 September, is presented. Suzaku observed IGR J17497-2821 on September 25, eight days after its discovery, for a net exposure of about 53 ks. During the Suzaku observation, IGR J17497-2821 is very bright, 2 × 1037erg s-1

2009 Publications of the Astronomical Society of Japan
Suzaku 8
X-Ray Studies of HESS J1837-069 with Suzaku and ASCA: a VHE Gamma-Ray Source Originated from the Pulsar Wind Nebula
DOI: 10.1093/pasj/61.sp1.S183 Bibcode: 2009PASJ...61S.183A

Dotani, Tadayasu; Ebisawa, Ken; Bamba, Aya +1 more

We present ASCA and Suzaku studies of the TeV source HESS J1837-069, which has not been identified in other wavelengths. We confirm the presence of two X-ray sources in the Suzaku XIS image, AX J1838.0-0655 and AX J1837.3-0652, near both ends of the elongated TeV emission region. The XIS spectra of the two sources were reproduced by an absorbed po…

2009 Publications of the Astronomical Society of Japan
Suzaku 7
Particle Propagation in the Galactic Center and Spatial Distribution of Non-Thermal X-Rays
DOI: 10.1093/pasj/61.5.1093 Bibcode: 2009PASJ...61.1093D

Maeda, Yoshitomo; Kokubun, Motohide; Nakazawa, Kazuhiro +9 more

We showed that if the non-thermal emission from the galactic center in the range 14-40 keV is due to inverse bremsstrahlung emission of subrelativistic protons, their interactions with hot and cold fractions of the interstellar medium are equally important. Our estimation shows that about 30% of the total non-thermal flux from the GC in the range …

2009 Publications of the Astronomical Society of Japan
Suzaku 6
Suzaku Observation of the Metallicity in the Interstellar Medium of NGC 4258
DOI: 10.1093/pasj/61.5.941 Bibcode: 2009PASJ...61..941K

Isobe, Naoki; Gandhi, Poshak; Sato, Kosuke +7 more

The Suzaku X-ray satellite observed the nearby spiral galaxy NGC 4258 for a total good exposure time of 100 ks. We present an analysis of the Suzaku XIS data, in which we confirm that the 0.5-2 keV spectra of the interstellar medium (ISM) are well-represented by a two-temperature model. The cool and hot ISM temperatures are 0.23±0.01 and 0.58±0.01…

2009 Publications of the Astronomical Society of Japan
Suzaku 6
High-Resolution Near-Infrared Images of the T Tauri Binary System XZ Tauri
DOI: 10.1093/pasj/61.6.1271 Bibcode: 2009PASJ...61.1271H

Pyo, Tae-Soo; Tamura, Motohide; Hayashi, Masahiko +8 more

We present a high-resolution (∼0.1'' = 14AU) H-band image of XZ Tau, a 0.3''-separated classical T Tauri binary system, taken with the Coronagraphic Imager with Adaptive Optics (CIAO) on the Subaru Telescope. We found a scattered light nebula extending to ∼2.4'' from the secondary, XZ Tau S, in the northeast region of the binary. Its surface brigh…

2009 Publications of the Astronomical Society of Japan
eHST 6
Suzaku Observations of SN 1987A
DOI: 10.1093/pasj/61.4.895 Bibcode: 2009PASJ...61..895S

Haberl, Frank; Hasinger, Günther; Sturm, Richard +2 more

We report on Suzaku observations of SN1987A in the Large Magellanic Cloud, performed in 2005 November and 2006 June. The observations provide medium resolution X-ray spectra during the phase of the interaction between the supernova blast wave and the inner circumstellar ring. The Suzaku observations complement XMM-Newton and Chandra observations a…

2009 Publications of the Astronomical Society of Japan
Suzaku XMM-Newton 6
AKARI Far-Infrared Spectroscopic Observations of the Galactic Center Region
DOI: 10.1093/pasj/61.3.511 Bibcode: 2009PASJ...61..511Y

Takahashi, H.; Nakagawa, T.; Okada, Y. +5 more

We have observed the Quintuplet- and Arches-cluster regions with the Fourier Transform Spectrometer (FTS) of the Far-Infrared Surveyor (FIS) aboard AKARI to investigate the physical conditions of interstellar matter around the clusters. The FIS-FTS mapping data reveal differences in the spatial distribution among the far-infrared [OIII], [NII], an…

2009 Publications of the Astronomical Society of Japan
AKARI ISO 5