scholarly journals Resolving the Formation of Cold H i Filaments in the High-velocity Cloud Complex C

2021 ◽  
Vol 921 (1) ◽  
pp. 11
Author(s):  
Antoine Marchal ◽  
Peter G. Martin ◽  
Munan Gong
2020 ◽  
Vol 902 (2) ◽  
pp. 154
Author(s):  
Kathleen A. Barger ◽  
David L. Nidever ◽  
Cannan Huey-You ◽  
Nicolas Lehner ◽  
Katherine Rueff ◽  
...  

2000 ◽  
Vol 538 (1) ◽  
pp. L35-L38 ◽  
Author(s):  
E. M. Murphy ◽  
K. R. Sembach ◽  
B. K. Gibson ◽  
J. M. Shull ◽  
B. D. Savage ◽  
...  

2004 ◽  
Vol 602 (2) ◽  
pp. 738-759 ◽  
Author(s):  
Andrew J. Fox ◽  
Blair D. Savage ◽  
Bart P. Wakker ◽  
Philipp Richter ◽  
Kenneth R. Sembach ◽  
...  

2018 ◽  
Vol 2 (2) ◽  
pp. 59
Author(s):  
J. E. G. Peek ◽  
Rongmon Bordoloi ◽  
Hugues Sana ◽  
Julia Roman-Duval ◽  
Jason Tumlinson ◽  
...  

2006 ◽  
Vol 638 (2) ◽  
pp. L97-L100 ◽  
Author(s):  
C. Thom ◽  
M. E. Putman ◽  
B. K. Gibson ◽  
N. Christlieb ◽  
C. Flynn ◽  
...  

2008 ◽  
Vol 684 (1) ◽  
pp. 364-372 ◽  
Author(s):  
C. Thom ◽  
J. E. G. Peek ◽  
M. E. Putman ◽  
Carl Heiles ◽  
K. M. G. Peek ◽  
...  

1989 ◽  
Vol 120 ◽  
pp. 458-458
Author(s):  
U. Herbstmeier

Examining the high velocity cloud complex C and its possible interaction with gas of the galactic disk we became aware of a dust cloud located at galactic longitude l = 86° and latitude b = 38°.5 seen in the l00µm image of the IRAS. This cloud consists of a cucumber shaped core surounded by a horseshoe shaped halo opening towards larger galactic coordinates. At very low 100µm intensities dust lanes starting at the core or the ends of the horseshoe can be traced for about 5° towards high galactic latitude and longitude.


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