Titlebook: Spatial Pattern in Plankton Communities; John H. Steele Book 1978 Springer Science+Business Media New York 1978 fields.nuclear physics.phy

mentor

書目名稱Spatial Pattern in Plankton Communities影響因子(影響力)




書目名稱Spatial Pattern in Plankton Communities影響因子(影響力)學(xué)科排名




書目名稱Spatial Pattern in Plankton Communities網(wǎng)絡(luò)公開(kāi)度




書目名稱Spatial Pattern in Plankton Communities網(wǎng)絡(luò)公開(kāi)度學(xué)科排名




書目名稱Spatial Pattern in Plankton Communities被引頻次




書目名稱Spatial Pattern in Plankton Communities被引頻次學(xué)科排名




書目名稱Spatial Pattern in Plankton Communities年度引用




書目名稱Spatial Pattern in Plankton Communities年度引用學(xué)科排名




書目名稱Spatial Pattern in Plankton Communities讀者反饋




書目名稱Spatial Pattern in Plankton Communities讀者反饋學(xué)科排名

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HERTZ

Akira Okubor techniques, such as photometric transit and microlensing surveys, have recently started to contribute to the planetary census. With ～130 host systems currently known, it is clear that the mass distribution of these very-low mass companions is not an extension of the mass function of stellar/brown

LARK

G. E. B. Kullenbergre parameters, such as the local mass density. At present, masses can be derived directly only for stars in binary systems with well-determined orbits, although microlensing projects may offer additional data in the future. Those stars are used to calibrate empirical mass-luminosity relationships, w

endure

Trevor Plattr techniques, such as photometric transit and microlensing surveys, have recently started to contribute to the planetary census. With ～130 host systems currently known, it is clear that the mass distribution of these very-low mass companions is not an extension of the mass function of stellar/brown

Insul島

Kenneth L. Denman,David L. Mackasp to test the effect of altering one specific variable, such as temperature, pressure or concentration. However, the physical conditions which pervade in most celestial objects are so extreme that there can be no question of their being matched in terrestrial laboratories, so direct experimentation

anesthesia

令人悲傷

M. J. R. Fashamllagher et al. (1984), who determined the SFR at three different epochs of galactic evolution. Sandage’s figure establishes a connection of SFR and Hubble type but, as was already mentioned by Sandage, it “contains no physics” In order to explore the background of this connection, however, it is nec

輕而薄

Geoffrey T. Evansave cuspy cores: at the “break radius”.. (formerly the core radius ..), the steep outer surface brightness profile turns down to a shallow inner power law ., .. The corresponding slope of the deprojected profile is derived; the flattest cores allow box orbits to survive. Cores continue to satisfy fu

誘惑

R. D. Pingreellagher et al. (1984), who determined the SFR at three different epochs of galactic evolution. Sandage’s figure establishes a connection of SFR and Hubble type but, as was already mentioned by Sandage, it “contains no physics” In order to explore the background of this connection, however, it is nec