output
20022026
most citedWeak localisation magnetoresistance and valley symmetry in graphene

954 citations

Showing 2008 · astro-phShow all

7 papers · 2 filters

astro-ph2008

Evolution of newly formed dust in Population III supernova remnants and its impact on the elemental composition of Population II.5 stars

Takaya Nozawa, Takashi Kozasa, Asao Habe +5

We investigate the evolution of dust formed in Population III supernovae (SNe) by considering its transport and processing by sputtering within the SN remnants (SNRs). We find that…

astro-ph2008★ 37 cited

An Eight-Octant Phase-Mask Coronagraph

N. Murakami, R. Uemura, N. Baba +4

We present numerical simulations and laboratory experiments on an eight-octant phase-mask (EOPM) coronagraph. The numerical simulations suggest that an achievable contrast for the…

astro-ph2008★ 7 cited

Microstructure and kinematics of H2O masers in the massive star forming region IRAS 06061+2151

K. Motogi, Y. Watanabe, K. Sorai +14

We have made multi-epoch VLBI observations of H2O maser emission in the massive star forming region IRAS 06061+2151 with the Japanese VLBI network (JVN) from 2005 May to 2007 Octob…

astro-ph2008★ 27 cited

Structural effects of ice grain surfaces on the hydrogenation of CO at low temperatures

H. Hidaka, N. Miyauchi, A. Kouchi +1

Experiments on the hydrogenation of CO on crystalline and amorphous ice at 15 K were carried out to investigate the structural effects of the ice surface. The effective rate of H a…

astro-ph2008★ 181 cited

Formation of hydrogen peroxide and water from the reaction of cold hydrogen atoms with solid oxygen at 10K

N. Miyauchi, H. Hidaka, T. Chigai +3

The reactions of cold H atoms with solid O2 molecules were investigated at 10 K. The formation of H2O2 and H2O has been confirmed by in-situ infrared spectroscopy. We found that th…

astro-ph2008★ 30 cited

Extinction curves flattened by reverse shocks in supernovae

Hiroyuki Hirashita, Takaya Nozawa, Tsutomu T. Takeuchi +1

We investigate the extinction curves of young galaxies in which dust is supplied from Type II supernovae (SNe II) and/or pair instability supernovae (PISNe). Since at high redshift…