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A Suzaku Observation of the Low-Ionization Fe-Line Emission from RCW 86
Masaru Ueno, Rie Sato, Jun Kataoka +14
The newly operational X-ray satellite Suzaku observed the southwestern quadrant of the supernova remnant (SNR) RCW 86 in February 2006 to study the nature of the 6.4 keV emission l…
Suzaku Observations of the Local and Distant Hot ISM
Randall K. Smith, Mark W. Bautz, Richard J. Edgar +18
Suzaku observed the molecular cloud MBM12 and a blank field less than 3 degrees away to separate the local and distant components of the diffuse soft X-ray background. Towards MBM1…
X-ray Spectral Study of the extended emission,'the Cap', located 11.6 kpc above the disk of M82
Takeshi Go Tsuru, Midori Ozawa, Yoshiaki Hyodo +11
The extended X-ray emission from 'the Cap' region located 11' (11.6 kpc) above the disk of the starburst galaxy M82 has been observed with Suzaku and XMM-Newton. Owing to the good…
An Apparent Hard X-ray Decline of CH Cygni
Koji Mukai, Manabu Ishida, Caroline Kilbourne +4
CH Cygni is a symbiotic star consisting of an M giant and an accreting white dwarf, which is known to be a highly variable X-ray source with a complex, two-component, spectra. Here…