Journal
ASTROPHYSICAL JOURNAL
Volume 726, Issue 2, Pages -Publisher
IOP PUBLISHING LTD
DOI: 10.1088/0004-637X/726/2/91
Keywords
ISM: bubbles; ISM: supernova remnants; solar wind; Sun: heliosphere; X-rays: diffuse background; X-rays: ISM
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Funding
- NASA [NAS5-00132]
- Goddard Space Flight Center
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We present the first analysis of an XMM-Newton observation of the nearby molecular cloud MBM 12. We find that in the direction of MBM 12 the total OVII (0.57 keV) triplet emission is 1.8(-0.6)(+0.5) photons cm(-2) s(-1) sr(-1) (or line units, LU) while for the OVIII (0.65 keV) line emission we find a 3 sigma upper limit of < 1 LU. We use a heliospheric model to calculate the OVII and OVIII emission generated by Solar Wind Charge-eXchange (SWCX) which we compare to the XMM-Newton observations. This comparison provides new constraints on the relative heliospheric and Local Bubble contributions to the local diffuse X-ray background. The heliospheric SWCX model predicts 0.82 LU for OVII, which accounts for similar to 46% +/- 15% of the observed value, and 0.33 LU for the OVIII line emission consistent with the XMM-Newton observed value. We discuss our results in combination with previous observations of MBM 12 with Chandra and Suzaku.
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