scholarly journals Attempt to detect diamagnetic anisotropy of dust-sized crystal orientated to investigate the origin of interstellar dust alignment

2013 ◽  
Vol 65 (3) ◽  
pp. 193-197 ◽  
Author(s):  
T. Takeuchi ◽  
K. Hisayoshi ◽  
C. Uyeda
Keyword(s):  
Interstellar Dust ◽  
Diamagnetic Anisotropy ◽  
Dust Alignment

Chemical evolution of interstellar dust, comets and the origins of life

1989 ◽  
Vol 14 (2) ◽  
pp. 103-131 ◽  
Author(s):  
J. Mayo Greenberg ◽  
Nansheng Zhao ◽  
Joniek Hage
Keyword(s):  
Chemical Evolution ◽  
Interstellar Dust ◽  
Origins Of Life

PRONAOS observations of the interstellar medium: New insights on interstellar Dust

2002 ◽  
Vol 4 ◽  
pp. 9-9
Author(s):  
I. Ristorcelli ◽  
B. Stepnik ◽  
X. Dupac ◽  
A. Abergel ◽  
J. P. Bernard ◽  
...  
Keyword(s):  
Interstellar Medium ◽  
Interstellar Dust

DIAMAGNETIC ANISOTROPY, ISOTOPE SHIFT AND COOLING-SPEED EFFECTS IN SUPERCONDUCTING (TMTSF)2C104CRYSTALS

1983 ◽  
Vol 44 (C3) ◽  
pp. C3-1041-C3-1045 ◽  
Author(s):  
H. Schwenk ◽  
K. Andres ◽  
F. Wudl ◽  
E. Aharon-Shalom
Keyword(s):  
Isotope Shift ◽  
Diamagnetic Anisotropy ◽  
Cooling Speed

Extinction Curves, Distances, and Clumpiness of Diffuse Interstellar Dust Clouds

1999 ◽  
Vol 117 (5) ◽  
pp. 2226-2243 ◽  
Author(s):  
Arpad Szomoru ◽  
Puragra Guhathakurta
Keyword(s):  
Interstellar Dust ◽  
Dust Clouds

Magnetic Properties of Liquid Crystals Incorporating Metal Centres

1989 ◽  
Vol 175 ◽  
Author(s):  
Wolfgang Haase ◽  
Stefan Gehring ◽  
Bettina Borchers
Keyword(s):  
Magnetic Properties ◽  
Magnetic Susceptibility ◽  
Liquid Crystals ◽  
Molecular Interactions ◽  
Magnetic Susceptibility Data ◽  
Susceptibility Data ◽  
Magnetic Effects ◽  
Diamagnetic Anisotropy

AbstractMagnetic susceptibility data (300–520 K) of monomeric and dimeric mesogenic copper(II) compounds are presented. Different magnetic effects arising from the paramagnetic Cu(II)-centres and the diamagnetic anisotropy of the mesogenic groups are observed and discussed with respect to possible inter molecular interactions.

A study of interstellar dust

Astrophysics ◽  
1969 ◽  
Vol 3 (4) ◽  
pp. 224-228
Author(s):  
I. N. Minin
Keyword(s):  
Interstellar Dust

Diamagnetic Anisotropy Measurements of Nematic Liquid Crystals

1986 ◽  
Vol 140 (2-4) ◽  
pp. 83-93 ◽  
Author(s):  
Shin-Tson Wu ◽  
Willis H. Smith ◽  
Anna M. Lackner
Keyword(s):  
Liquid Crystals ◽  
Nematic Liquid Crystals ◽  
Diamagnetic Anisotropy

Temperature fluctuations in interstellar dust grains

1979 ◽  
Vol 65 (1) ◽  
pp. 155-166 ◽  
Author(s):  
Per A. Aannestad ◽  
Scott J. Kenyon
Keyword(s):  
Interstellar Dust ◽  
Temperature Fluctuations ◽  
Dust Grains ◽  
Interstellar Dust Grains

scholarly journals DIBs, Interstellar Dust, and Extinction

2013 ◽  
Vol 9 (S297) ◽  
pp. 147-152 ◽  
Author(s):  
G. C. Clayton
Keyword(s):  
Interstellar Medium ◽  
Interstellar Dust ◽  
Dust Grains ◽  
Weak Correlation ◽  
Interstellar Clouds ◽  
The Galaxy ◽  
The Relationship

AbstractThe relationship between DIBs and dust is still unknown. The correlation between reddening and DIB strength means that the DIBs are mixed in with the dust and gas in interstellar clouds. The DIBs are relatively stronger in the diffuse interstellar medium than in dense clouds. There is only a weak correlation between the DIBs and the UV extinction parameters including the 2175 Å bump strength and the far-UV rise. In addition, the bump dust grains are sometimes polarized, while the DIBs are not. However, observations of DIBs in the SMC show that when the 2175 Å bump is weak or missing so are the DIBs. Two of the four sightlines that deviate strongly from the CCM UV extinction in the Galaxy show weak DIBs.

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