scholarly journals Small‐Scale Structure at High Redshift. IV. Low‐Ionization Gas Intersecting Three Lines of Sight to Q2237+0305

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

scholarly journals Small‐Scale Structure at High Redshift. II. Physical Properties of the CivAbsorbing Clouds

2001 ◽  
Vol 554 (2) ◽  
pp. 823-840 ◽  
Author(s):  
Michael Rauch ◽  
Wallace L. W. Sargent ◽  
Thomas A. Barlow
Keyword(s):  
Physical Properties ◽  
High Redshift ◽  
Scale Structure ◽  
Small Scale ◽  
Small Scale Structure

scholarly journals Small‐Scale Structure at High Redshift. I. Glimpses of the Interstellar Medium at Redshift ∼3.5

1999 ◽  
Vol 515 (2) ◽  
pp. 500-505 ◽  
Author(s):  
Michael Rauch ◽  
Wallace L. W. Sargent ◽  
Tom A. Barlow
Keyword(s):  
Interstellar Medium ◽  
High Redshift ◽  
Scale Structure ◽  
Small Scale ◽  
Small Scale Structure

scholarly journals Small Scale Structure and High Redshift HI

1996 ◽  
pp. 93-107 ◽  
Author(s):  
David H. Weinberg ◽  
Lars Hernquist ◽  
Neal S. Katz ◽  
Jordi Miralda-Escudé
Keyword(s):  
High Redshift ◽  
Scale Structure ◽  
Small Scale ◽  
Small Scale Structure

scholarly journals Small‐Scale Structure at High Redshift. III. The Clumpiness of the Intergalactic Medium on Subkiloparsec Scales

2001 ◽  
Vol 562 (1) ◽  
pp. 76-87 ◽  
Author(s):  
Michael Rauch ◽  
Wallace L. W. Sargent ◽  
Thomas A. Barlow ◽  
Robert F. Carswell
Keyword(s):  
Intergalactic Medium ◽  
High Redshift ◽  
Scale Structure ◽  
Small Scale ◽  
Small Scale Structure

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
Keyword(s):  
High Redshift ◽  
Scale Structure ◽  
Small Scale ◽  
Small Scale Structure

scholarly journals A Search for Very Compact Structure in 17 OH Masers

1988 ◽  
Vol 129 ◽  
pp. 255-256
Author(s):  
A. J. Kemball ◽  
P. J. Diamond ◽  
F. Mantovani
Keyword(s):  
Galactic Disk ◽  
Hii Regions ◽  
Scale Structure ◽  
Small Scale ◽  
Compact Structure ◽  
Small Scale Structure ◽  
Interstellar Scattering

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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