Publication Year: 1963
DOI: https://doi.org/10.1039/jr9630000479
Abstract: R. J. Pierens, J. Chem. Soc., 1963, 479 DOI: 10.1039/JR9630000479 W. Le Fèvre, A. Sundaram and R. K.
Authors:
Publication Year: 2017
DOI: https://doi.org/10.1177/1528083717725912
Abstract: Corduroy fabrics This the acoustic absorption coefficient of corduroy fabric, and the difference work of acoustic absorption is due to the varied air permeability mainly and airflow resistance resulting from the different wale width. investigated the acoustical properties of corduroy fabrics have in relation to air permeability and airflow resistance. Show more
Authors:
Publication Year: 2018
DOI: https://doi.org/10.1121/1.5049708
Abstract: Both specific as that those predicted from the air permeability are more accurate a than those from the measured specific airflow resistance for textiles. parameter to estimate the sound absorption of textiles. airflow The measurement of specific airflow resistance is specified in ISO resistance 9053 (Int. Standards Org., 1991), but Show more
Authors:
Publication Year: 2005
DOI: https://doi.org/10.1086/428769
Abstract: We demonstrate to compute the gravitational potential and field in the plane the of razor-thin, axially symmetric discs, as preliminarily outlined in Pierens high & Hure (2004). Because residual kernels in Poisson integrals are accuracy not C^infinity-class functions, we use a dynamical space mapping in of order to increase the Show more
Authors:
Publication Year: 2009
DOI: https://doi.org/10.1111/j.1365-2966.2009.15107.x
Abstract: This paper Pierens possibility of their resonant locking. However, in the case in & which the gas giant has the mass of Jupiter, before Nelson any mean motion first order commensurability could be achieved, the (2008) Super-Earth is caught in a trap when it is very in close to the Show more
Authors:
Publication Year: 2010
DOI: DOI not available
Abstract: A new meeting) conditions (see, eg. Raymond et al. 2009). Additionally, the outward explores migration of the giant planets populates the asteroid belt with the distinct populations of bodies, with the inner belt filled by effects bodies originating inside of 3 AU, and the outer belt of filled with bodies Show more
Authors:
Publication Year: 2017
DOI: https://doi.org/10.1016/j.icarus.2017.06.030
Abstract: Not available
Authors:
Publication Year: 1981
DOI: https://doi.org/10.1016/0009-2614(81)85228-1
Abstract: Not available
Authors:
Publication Year: 1973
DOI: https://doi.org/10.1063/1.1680745
Abstract: Views Icon Supplementary Search Advanced Search |Citation Search Data Peer Review Share Icon Share Twitter Facebook Reddit Views LinkedIn Tools Icon Tools Reprints and Permissions Cite Icon Cite Article Search Site Citation C. L. Cheng, R. K. Pierens, D. contents V. Radford, G. L. D. Ritchie; Structure of mercury(II) chloride Show more
Authors:
Publication Year: 2011
DOI: https://doi.org/10.1088/0004-637x/729/1/47
Abstract: We use whether fewer planets can also generate a large cavity interior to dynamically-interacting the locally formed gap(s) by preventing outer disk material from multiple moving in. In these cases, however, the reduction of surface giant density produces a corresponding reduction in the inner disk accretion planets rate onto the Show more
Authors:
Publication Year: 2017
DOI: https://doi.org/10.1093/mnras/stx1232
Abstract: 'Hot super-Earths' size chains are far more compact than the observed super-Earth systems. with Once the gas dissipates, resonant chains may become dynamically unstable. period They undergo a phase of giant impacts that spreads the shorter systems out. Disc turbulence has no measurable effect on the than outcome. Our simulations Show more
Authors:
Publication Year: 2012
DOI: https://doi.org/10.1088/0004-6256/144/4/117
Abstract: Several properties spacing can be avoided if the mass of the transplanetary disk and of planetesimals was large (Mdisk ≳ 50 MEarth), but we orbital found that a massive disk would lead to excessive dynamical eccentricities damping (e.g., final e55 ≲ 0.01 compared to present e55 of = 0.044, where Show more
Authors:
Publication Year: 2011
DOI: https://doi.org/10.1088/2041-8205/742/2/l22
Abstract: Studies of giant dynamical simulations starting with a resonant system of four giant planets planets have a low success rate in matching the present formed orbits of giant planets and various other constraints (e.g., survival and of the terrestrial planets). The dynamical evolution is typically too migrated violent, if Jupiter Show more
Authors:
Publication Year: 2015
DOI: DOI not available
Abstract: Not available
Authors:
Publication Year: 1999
DOI: DOI not available
Abstract: Not available
Authors:
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