Small‐Scale Structure in the Lyα Forest at High Redshift

1998 ◽  
Vol 494 (1) ◽  
pp. 60-89 ◽  
Author(s):  
C. E. Petry ◽  
C. D. Impey ◽  
C. B. Foltz
2001 ◽  
Vol 554 (2) ◽  
pp. 823-840 ◽  
Author(s):  
Michael Rauch ◽  
Wallace L. W. Sargent ◽  
Thomas A. Barlow

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

Author(s):  
David H. Weinberg ◽  
Lars Hernquist ◽  
Neal S. Katz ◽  
Jordi Miralda-Escudé

2001 ◽  
Vol 562 (1) ◽  
pp. 76-87 ◽  
Author(s):  
Michael Rauch ◽  
Wallace L. W. Sargent ◽  
Thomas A. Barlow ◽  
Robert F. Carswell

2002 ◽  
Vol 576 (1) ◽  
pp. 45-60 ◽  
Author(s):  
Michael Rauch ◽  
Wallace L. W. Sargent ◽  
Thomas A. Barlow ◽  
Robert A. Simcoe

1988 ◽  
Vol 129 ◽  
pp. 255-256
Author(s):  
A. J. Kemball ◽  
P. J. Diamond ◽  
F. Mantovani

The apparent spot sizes of OH masers appear to be significantly broadened when seen through the inner galaxy or large extents of the galactic disk (Burke 1968). Bowers et al (1980) found evidence of small-scale structure (≲ 50 mas) in OH sources at distances of less than 5 kpc but this was characteristically absent in very distant sources (≳ 8kpc) at galactic longitudes 1 ≲ 40°. This result is typically explained in terms of interstellar scattering (ISS) by intervening diffuse HII regions.


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