Search Publications

A Time-Variable X-Ray Echo: Indications of a Past Flare of the Galactic-Center Black Hole
DOI: 10.1093/pasj/60.sp1.S201 Bibcode: 2008PASJ...60S.201K

Koyama, Katsuji; Matsumoto, Hironori; Tsuru, Takeshi Go +1 more

A time-variability study of the neutral iron line flux at 6.40keV in the Sgr B2 region from data of Suzaku and Chandra is presented. The highly ionized iron line at 6.68keV is due to Galactic Center Diffuse X-rays, and is thus time invariable. By comparing the 6.68keV and 6.40keV line fluxes, we found that the 6.40keV flux from the Sgr B2 complex …

2008 Publications of the Astronomical Society of Japan
Suzaku 44
Spectral Study of the Galactic Ridge X-Ray Emission with Suzaku
DOI: 10.1093/pasj/60.sp1.S223 Bibcode: 2008PASJ...60S.223E

Tsujimoto, Masahiro; Kokubun, Motohide; Koyama, Katsuji +7 more

In order to carry out a precise spectral study of the Galactic Ridge X-ray Emission using Suzaku, we have observed a typical Galactic plane field at (l,b) = (28°46, -0°20), which is already deeply observed with Chandra, and known to be devoid of bright X-ray point sources. Thanks to the low background and high spectral resolution of Suzaku, we wer…

2008 Publications of the Astronomical Society of Japan
Suzaku 44
Measuring the Broad-Band X-Ray Spectrum from 400eV to 40keV in the Southwest Part of the Supernova Remnant RXJ1713.7-3946
DOI: 10.1093/pasj/60.sp1.S131 Bibcode: 2008PASJ...60S.131T

Petre, Robert; Kokubun, Motohide; Nakazawa, Kazuhiro +13 more

We report on results from Suzaku broadband X-ray observations of the southwest part of the galactic supernova remnant (SNR) RXJ1713.7-3946 with an energy coverage of 0.4-40keV. The X-ray spectrum, presumably of synchrotron origin, is known to be completely lineless, making this SNR ideally suited for a detailed study of the X-ray spectral shape fo…

2008 Publications of the Astronomical Society of Japan
Suzaku 43
Suzaku Spectroscopy of an X-Ray Reflection Nebula and a New Supernova Remnant Candidate in the SgrB1 Region
DOI: 10.1093/pasj/60.sp1.S191 Bibcode: 2008PASJ...60S.191N

Koyama, Katsuji; Nakajima, Hiroshi; Matsumoto, Hironori +7 more

We made a 100 ks observation of the Sagittarius (Sgr) B1 region at (l, b) = (0°.5, -0°.1) near to the Galactic center (GC) with the Suzaku/XIS. Emission lines of SXV, FeI, FeXXV, and FeXXVI were clearly detected in the spectrum. We found that the FeXXV and FeXXVI line emissions smoothly distribute over the SgrB1 and B2 regions connecting from the …

2008 Publications of the Astronomical Society of Japan
Suzaku 41
In-Orbit Timing Calibration of the Hard X-Ray Detector on Board Suzaku
DOI: 10.1093/pasj/60.sp1.S25 Bibcode: 2008PASJ...60S..25T

Dotani, Tadayasu; Enoto, Teruaki; Yamaoka, Kazutaka +28 more

The hard X-ray detector (HXD) aboard the X-ray satellite Suzaku is designed to have a good timing capability with a 61µs time resolution. In addition to detailed descriptions of the HXD timing system, results of in-orbit timing calibration and the performance of the HXD are summarized. The relative accuracy of time measurements of the HXD ev…

2008 Publications of the Astronomical Society of Japan
INTEGRAL Suzaku 41
Suzaku Observations of the North Polar Spur: Evidence for Nitrogen Enhancement
DOI: 10.1093/pasj/60.sp1.S95 Bibcode: 2008PASJ...60S..95M

Miller, Eric D.; Katsuda, Satoru; Kokubun, Motohide +10 more

We present observations of the North Polar Spur (NPS) using the X-ray Imaging Spectrometer (XIS) aboard the Suzaku X-ray satellite. The NPS is a large region of enhanced soft X-ray and radio emission projected above the plane of the Galaxy, likely produced by a series of supernovae and stellar winds from the nearby Sco-Cen OB association. The exce…

2008 Publications of the Astronomical Society of Japan
Suzaku 41
Hinode's Observational Result on the Saturation of Magnetic Helicity Injected into the Solar Atmosphere and Its Relation to the Occurrence of a Solar Flare
DOI: 10.1093/pasj/60.5.1181 Bibcode: 2008PASJ...60.1181M

Magara, Tetsuya; Tsuneta, Saku

This paper is intended to present key features of the evolution toward the onset of a solar flare, using Hinode's observations on the photospheric magnetic field. Hinode can provide the temporal development of the photospheric field as a vector quantity, which shows that magnetic shear is initially developed in a flare-productive active region (AR…

2008 Publications of the Astronomical Society of Japan
Hinode 41
VLBI Astrometry of AGB Variables with VERA --- A Semiregular Variable S Crateris ---
DOI: 10.1093/pasj/60.5.1013 Bibcode: 2008PASJ...60.1013N

Hirota, Tomoya; Kurayama, Tomoharu; Honma, Mareki +40 more

We present a distance measurement for the semiregular variable S Crateris (S Crt) based on its annual parallax. With the unique dual beam system of the VLBI Exploration for Radio Astrometry (VERA) telescopes, we measured the absolute proper motion of a water maser spot associated with S Crt, referred to the quasar J1147-0724 located at an angular …

2008 Publications of the Astronomical Society of Japan
Hipparcos 40
Suzaku Observations of Hercules X-1: Measurements of the Two Cyclotron Harmonics
DOI: 10.1093/pasj/60.sp1.S57 Bibcode: 2008PASJ...60S..57E

Dotani, Tadayasu; Enoto, Teruaki; Kokubun, Motohide +10 more

The accretion-powered pulsar Her X-1 was observed with Suzaku twice in its main-on state, on 2005 October 5--6 and 2006 March 29--30, for a net exposure of 30.5ks and 34.4ks, respectively. In the 2005 and 2006 observations, the source was detected at an average 10--30keV intensity of 290mCrab and 230mCrab, respectively. The intrinsic pulse period …

2008 Publications of the Astronomical Society of Japan
Suzaku 39
Wide-Band Spectroscopy of the Compton Thick Seyfert2 Galaxy Markarian 3 with Suzaku
DOI: 10.1093/pasj/60.sp1.S293 Bibcode: 2008PASJ...60S.293A

Isobe, Naoki; Kunieda, Hideyo; Okajima, Takashi +15 more

We obtained a wide-band spectrum of the Compton-thick Seyfert2 galaxy Mkn3 with Suzaku. The observed spectrum was clearly resolved into weak, soft power-law emission, a heavily absorbed power-law component, cold reflection, and many emission lines. The heavily absorbed component, absorbed by gas with a column density of 1.1 × 1024 cm

2008 Publications of the Astronomical Society of Japan
Suzaku 33