scholarly journals A comparison of the UV and HI properties of the extended UV (XUV) disk galaxies NGC 2541, NGC 5832 and ESO406-042

2021 ◽  
Vol 42 (2) ◽  
Author(s):  
M. Das ◽  
J. Yadav ◽  
N. Patra ◽  
K. S. Dwarakanath ◽  
S. S. McGaugh ◽  
...  
Keyword(s):  
1967 ◽  
Vol 31 ◽  
pp. 313-317 ◽  
Author(s):  
C. C. Lin ◽  
F. H. Shu

Density waves in the nature of those proposed by B. Lindblad are described by detailed mathematical analysis of collective modes in a disk-like stellar system. The treatment is centered around a hypothesis of quasi-stationary spiral structure. We examine (a) the mechanism for the maintenance of this spiral pattern, and (b) its consequences on the observable features of the galaxy.


2003 ◽  
Vol 10 ◽  
pp. 95-95
Author(s):  
E. Ardi ◽  
T. Tsuchiya ◽  
A. Burkert

2000 ◽  
Vol 119 (4) ◽  
pp. 1638-1644 ◽  
Author(s):  
J. A. L. Aguerri ◽  
A. M. Varela ◽  
M. Prieto ◽  
C. Muñoz-Tuñón

1997 ◽  
Vol 476 (2) ◽  
pp. 544-559 ◽  
Author(s):  
M. Samland ◽  
G. Hensler ◽  
Ch. Theis

2016 ◽  
Vol 25 (3) ◽  
Author(s):  
E. O. Vasiliev ◽  
S. A. Khoperskov ◽  
A. V. Khoperskov

AbstractWe use


2005 ◽  
Vol 627 (1) ◽  
pp. L17-L20 ◽  
Author(s):  
Jeremy Bailin ◽  
Daisuke Kawata ◽  
Brad K. Gibson ◽  
Matthias Steinmetz ◽  
Julio F. Navarro ◽  
...  

2000 ◽  
Vol 533 (1) ◽  
pp. 162-171 ◽  
Author(s):  
Habib G. Khosroshahi ◽  
Yogesh Wadadekar ◽  
Ajit Kembhavi
Keyword(s):  

2012 ◽  
Vol 756 (1) ◽  
pp. 30 ◽  
Author(s):  
Fazeel Mahmood Khan ◽  
Ingo Berentzen ◽  
Peter Berczik ◽  
Andreas Just ◽  
Lucio Mayer ◽  
...  

2006 ◽  
Vol 2 (S235) ◽  
pp. 143-143
Author(s):  
Eduard Vorobyov ◽  
Christian Theis

The majority of normal disk galaxies are characterized by non-axisymmetric structures like spirals or bars. These structural elements have been widely discussed in the literature as a result of gravitational instabilities which are connected to growing density waves or global instabilities of disks. A first insight into the properties of galactic discs was provided by linear stability analysis. However, a disadvantage of linear stability analysis remained its restriction to small perturbations, both in amplitude and wavelength. Thus, numerical simulations, especially hydrodynamical and stellar-hydrodynamical simulations became a primary tool for the analysis of galactic evolution.


2014 ◽  
Vol 148 (5) ◽  
pp. 77 ◽  
Author(s):  
Stacy S. McGaugh ◽  
James M. Schombert
Keyword(s):  

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