Plastics � Elasticity index � Determination of elastic property of melts

2021 ◽  
Keyword(s):  
Elastic Property

scholarly journals Characterization and Determination of Elastic Property of High-Density Nanocrystalline Gold Prepared by Gas-Deposition Method

2003 ◽  
Vol 44 (1) ◽  
pp. 94-103 ◽  
Author(s):  
Hisanori Tanimoto ◽  
Seiji Sakai ◽  
Eiji Kita ◽  
Hiroshi Mizubayashi
Keyword(s):  
Elastic Property ◽  
High Density ◽  
Deposition Method

Elastic property determination of nanostructured W/Cu multilayer films on a flexible substrate

2019 ◽  
Vol 35 (6) ◽  
pp. 1210-1216 ◽  
Author(s):  
Wei He ◽  
Meidong Han ◽  
Shibin Wang ◽  
Philippe Goudeau ◽  
Eric Le Bourhis ◽  
...  
Keyword(s):  
Elastic Property ◽  
Flexible Substrate ◽  
Multilayer Films

Galactic orbits of stars

1966 ◽  
Vol 25 ◽  
pp. 93-97
Author(s):  
Richard Woolley
Keyword(s):  
Globular Cluster ◽  
Potential Field ◽  
High Velocity ◽  
Velocity Vector ◽  
Variable Stars ◽  
The Sun ◽  
Proper Motions ◽  
Rr Lyrae ◽  
The Galaxy

It is now possible to determine proper motions of high-velocity objects in such a way as to obtain with some accuracy the velocity vector relevant to the Sun. If a potential field of the Galaxy is assumed, one can compute an actual orbit. A determination of the velocity of the globular clusterωCentauri has recently been completed at Greenwich, and it is found that the orbit is strongly retrograde in the Galaxy. Similar calculations may be made, though with less certainty, in the case of RR Lyrae variable stars.

Distance to SN 1987A and the LMC

1999 ◽  
Vol 190 ◽  
pp. 549-554
Author(s):  
Nino Panagia
Keyword(s):  
Angular Size ◽  
Large Magellanic Cloud ◽  
Magellanic Cloud ◽  
Light Curves ◽  
Distance Modulus ◽  
Absolute Size ◽  
Sn 1987A

Using the new reductions of the IUE light curves by Sonneborn et al. (1997) and an extensive set of HST images of SN 1987A we have repeated and improved Panagia et al. (1991) analysis to obtain a better determination of the distance to the supernova. In this way we have derived an absolute size of the ringRabs= (6.23 ± 0.08) x 1017cm and an angular sizeR″ = 808 ± 17 mas, which give a distance to the supernovad(SN1987A) = 51.4 ± 1.2 kpc and a distance modulusm–M(SN1987A) = 18.55 ± 0.05. Allowing for a displacement of SN 1987A position relative to the LMC center, the distance to the barycenter of the Large Magellanic Cloud is also estimated to bed(LMC) = 52.0±1.3 kpc, which corresponds to a distance modulus ofm–M(LMC) = 18.58±0.05.

Sign in / Sign up

Export Citation Format

Share Document