Suzaku Observations of the Local and Distant Hot ISM

Suzaku observed the molecular cloud MBM 12 and a blank field less than $3^{\circ}$ away to separate the local and distant components of the diffuse soft X-ray background. Towards MBM 12, a local ( $D \lesssim 275 \,\mathrm{pc}$ ) O VII emission line was clearly detected with an intensity of $3.5 \;\...

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Veröffentlicht in:Publications of the Astronomical Society of Japan 2007-01, Vol.59 (sp1), p.S141-S150
Hauptverfasser: Smith, Randall K., Bautz, Mark W., Edgar, Richard J., Fujimoto, Ryuichi, Hamaguchi, Kenji, Hughes, John P., Ishida, Manabu, Kelley, Richard, Kilbourne, Caroline A., Kuntz, K. D., McCammon, Dan, Miller, Eric, Mitsuda, Kazuhisa, Mukai, Koji, Plucinsky, Paul P., Porter, F. Scott, Snowden, Steve L., Takei, Yoh, Terada, Yukikatsu, Tsuboi, Yohko, Yamasaki, Noriko Y.
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Sprache:eng
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Zusammenfassung:Suzaku observed the molecular cloud MBM 12 and a blank field less than $3^{\circ}$ away to separate the local and distant components of the diffuse soft X-ray background. Towards MBM 12, a local ( $D \lesssim 275 \,\mathrm{pc}$ ) O VII emission line was clearly detected with an intensity of $3.5 \;\mathrm{photons} \;\mathrm{cm}^{-2} \,\mathrm{s}^{-1} \,\mathrm{sr}^{-1}$ (or line units, LU), and the O VIII flux was ${
ISSN:0004-6264
2053-051X
DOI:10.1093/pasj/59.sp1.S141