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20022009
most citedMeasuring the cosmic ray acceleration efficiency of a supernova remnant

171 citations · 435 across the 11 of their papers we have counts for

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astro-ph.GA2009171 cited

Measuring the cosmic ray acceleration efficiency of a supernova remnant

E. A. Helder, J. Vink, C. G. Bassa +7

Cosmic rays are the most energetic particles arriving at earth. Although most of them are thought to be accelerated by supernova remnants, the details of the acceleration process a…

astro-ph.HE2009

Line and Continuum Emission from the Galactic Center. III. Origin of 6.4 keV Line Emission from Molecular Clouds in the Galactic Center

Vladimir Dogiel, Kwong-Sang Cheng, Dmitrii Chernyshov +8

We analyze the 6.4 keV line and continuum emission from the molecular cloud Sgr B2 and the source HESS J1745-303, which is supposed to be a complex of molecular gas. From the HESS…

astro-ph.HE20096 cited

An Antarctic ice core recording both supernovae and solar cycles

Yuko Motizuki, Kazuya Takahashi, Kazuo Makishima +8

Ice cores are known to be rich in information regarding past climates, and the possibility that they record astronomical phenomena has also been discussed. Rood et al. were the fir…

astro-ph.HE200919 cited

Doppler-Broadened Iron X-ray Lines from Tycho's Supernova Remnant

A. Furuzawa, D. Ueno, A. Hayato +13

We use \suzaku observations to measure the spatial variation of the Fe K line with radius in the \tycho supernova remnant. The Fe line widths show a significant decrease from a…

astro-ph.IM2009

Modeling and Reproducibility of Suzaku HXD PIN/GSO Background

Yasushi Fukazawa, Tsunefumi Mizuno, Shin Watanabe +26

Suzaku Hard X-ray Detector (HXD) achieved the lowest background level than any other previously or currently operational missions sensitive in the energy range of 10--600 keV, by u…