San Francisco / Osaka / Taipei / Nagoya / Wiley / /
Company
Special Coordination Funds / The star / /
Country
Taiwan / Japan / / /
Event
Man-Made Disaster / /
Facility
Japan Sinica Institute / Nagoya University / Osaka Sangyo University / /
IndustryTerm
gas eff / spectral energy distribution / spectral energy distributions / metal mass / galaxy spectral energy distributions / chemical evolution / chemical evolution model / metal enrichment / metal / dMd gas / dust-to-gas mass ratio / metal abundance / dust-to-metal ratio / dust-to-gas / metal masses / dust-to-gas ratio / dust-to-gas mass ratio increases / clumpy media / gas phase / explosion energy / /
MusicAlbum
Culture / Technology / Sports / Science / /
Organization
Seismological Society of Japan / Japan Sinica Institute for Astronomy and Astrophysics / International Monetary Fund / Nagoya University / Geodetic Society of Japan / Japanese Society for Planetary Sciences / Department of Particle and Astrophysical Science / Scientific Research Fund / Volcanological Society of Japan / Ministry of Education / Osaka Sangyo University / Astronomical Society of the Pacific / Society of Geomagnetism and Earth / /
Person
R. Astron / L. Jiang / Daisuke Yamasawa / A. G. G. M. Tielens / D. J. Benford / K. M. Menten / D. J. Hollenbach / L. Allamandora / F. Matteucci / Takaya Nozawa / M. A. Strauss / G. Granato / J. A. Nuth / III / X. L. Fan / R. Maiolino / Gordon / C. L. Carilli / X. Fan / Takako T. Ishii / C. F. McKee / A. Kov´acs / A. Pipino / C. D. Dowell / F. Calura / Asao Habe / E. Giovannoli / V / L. Silva / Takashi Kozasa / A. Omont / Witt / F. Bertoldi / P. Cox / /
Position
driver / simple collapse model / General Education / representative / /
Earth Planets Space, 65, 213–222, 2013 Dust formation history of galaxies: A critical role of metallicity∗ for the dust mass growth by accreting materials in the interstellar medium Ryosuke S. Asano1 , Tsutomu T. Ta