139 citations · 391 across the 6 of their papers we have counts for
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astro-ph.GA2013★ 55 cited
Non-thermal X-rays and interstellar gas toward the γ-ray supernova remnant RX J1713.7-3946: Evidence for X-ray enhancement around CO and HI clumps
H. Sano, T. Tanaka, K. Torii +18
RX J1713.7-3946 is the most remarkable very-high-energy γ-ray supernova remnant which emits synchrotron X-rays without thermal features. We made a comparative study of CO, HI and X…
astro-ph.GA2011★ 139 cited
A Detailed Study of the Molecular and Atomic Gas Toward the γ-ray SNR RX J1713.7-3946: Spatial TeV γ-ray and ISM Gas Correspondence
Y. Fukui, H. Sano, J. Sato +14
RX J1713.73946 is the most remarkable TeV -ray SNR which emits -rays in the highest energy range. We made a new combined analysis of CO and \ion{H}{1} in the SNR and deriv…
astro-ph.GA2010★ 80 cited
Star Forming Dense Cloud Cores in the TeV γ-ray SNR RX J1713.7-3946
H. Sano, J. Sato, H. Horachi +23
RX J1713.7-3946 is one of the TeV γ-ray supernova remnants (SNRs) emitting synchrotron X rays. The SNR is associated with molecular gas located at ~1 kpc. We made new molecular obs…