scholarly journals   Orionis: further temporal variability and evidence for small-scale structure in the interstellar medium

2001 ◽  
Vol 321 (3) ◽  
pp. 553-558 ◽  
Author(s):  
R. J. Price ◽  
I. A. Crawford ◽  
I. D. Howarth
2006 ◽  
Vol 133 ◽  
pp. 403 ◽  
Author(s):  
Martin A. Cordiner ◽  
Stephen J. Fossey ◽  
Arfon M. Smith ◽  
Peter J. Sarre

2009 ◽  
Vol 53 (10) ◽  
pp. 879-885
Author(s):  
I. A. Mizeva ◽  
D. D. Sokoloff ◽  
A. Fletcher ◽  
P.G. Frick ◽  
A. Shukurov

1999 ◽  
Vol 515 (2) ◽  
pp. 500-505 ◽  
Author(s):  
Michael Rauch ◽  
Wallace L. W. Sargent ◽  
Tom A. Barlow

2013 ◽  
Vol 764 (1) ◽  
pp. L10 ◽  
Author(s):  
M. A. Cordiner ◽  
S. J. Fossey ◽  
A. M. Smith ◽  
P. J. Sarre

1985 ◽  
Vol 106 ◽  
pp. 311-317
Author(s):  
John M. Dickey

The interstellar medium shows turbulence whose velocity and density spectra are surprisingly like a Kolmogoroff law, in spite of the fact that the turbulence is generated mainly by microscopic explosions, rather than a cascade of energy from larger to smaller scales.


2003 ◽  
Vol 597 (1) ◽  
pp. 399-407 ◽  
Author(s):  
Joel N. Bregman ◽  
Megan C. Novicki ◽  
Jessica E. Krick ◽  
John S. Arabadjis

2012 ◽  
Vol 429 (2) ◽  
pp. 939-953 ◽  
Author(s):  
Keith T. Smith ◽  
Stephen J. Fossey ◽  
Martin A. Cordiner ◽  
Peter J. Sarre ◽  
Arfon M. Smith ◽  
...  

2013 ◽  
Vol 9 (S297) ◽  
pp. 141-143
Author(s):  
K. T. Smith ◽  
M. A. Cordiner ◽  
P. J. Sarre

AbstractWe present observations which probe the small-scale structure of the interstellar medium using diffuse interstellar bands (DIBs). Towards HD 168075/6 in the Eagle Nebula, significant differences in DIB absorption are found between the two lines of sight, which are separated by 0.25 pc, and λ 5797 exhibits a velocity shift. Similar data are presented for four stars in the μ Sgr system. We also present a search for variations in DIB absorption towards κ Vel, where the atomic lines are known to vary on scales of ~ 10 AU. Observations separated by ~ 9 yr yielded no evidence for changes in DIB absorption strength over this scale, but do reveal an unusual DIB spectrum.


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