scholarly journals IRAC Observations of COJ= 4 → 3 High‐Velocity Cloud in the 30 Doradus Complex in the Large Magellanic Cloud

2007 ◽  
Vol 669 (2) ◽  
pp. 1003-1010 ◽  
Author(s):  
Hak‐Sub Kim ◽  
Sungeun Kim ◽  
Jih‐Yong Bak ◽  
Mario Garcia ◽  
Bernard Brandl ◽  
...  
2005 ◽  
Vol 130 (4) ◽  
pp. 1635-1639 ◽  
Author(s):  
Sungeun Kim ◽  
Wilfred Walsh ◽  
Kecheng Xiao ◽  
Adair P. Lane

1980 ◽  
Vol 4 (1) ◽  
pp. 90-92
Author(s):  
P. J. McGregor ◽  
A. R. Hyland

The 30 Doradus region offers an excellent opportunity to study cluster formation processes and recent star formation in the Large Magellanic Cloud.


2003 ◽  
Vol 20 (3) ◽  
pp. 263-269 ◽  
Author(s):  
Daisuke Kawata ◽  
Christopher Thom ◽  
Brad K. Gibson

AbstractWe test the hypothesis that high-velocity gas cloud Complex C is actually a high-latitude spiral arm extension in the direction of the Galactic warp, as opposed to the standard interpretation — that of a once extragalactic, but now infalling, gas cloud. A parallel Tree N-body code was employed to simulate the tidal interaction of a satellite perturber with the Milky Way. We find that a model incorporating a perturber of the mass of the Large Magellanic Cloud on a south to north polar orbit, crossing the disk at ˜15 kpc, does yield a high-velocity, high-latitude extension consistent with the spatial, kinematical, and column density properties of Complex C. Unless this massive satellite remains undiscovered because of either a fortuitous alignment with the Galactic bulge (feasible within the framework of the model), or the lack of any associated baryonic component, we conclude that this alternative interpretation appears unlikely.


2009 ◽  
Vol 5 (S266) ◽  
pp. 35-40 ◽  
Author(s):  
C. J. Evans ◽  
N. Bastian ◽  
Y. Beletsky ◽  
I. Brott ◽  
M. Cantiello ◽  
...  

AbstractThe Tarantula Survey is an ambitious ESO Large Programme that has obtained multi-epoch spectroscopy of over 1000 massive stars in the 30 Doradus region in the Large Magellanic Cloud. Here, we introduce the scientific motivations of the survey and give an overview of the observational sample. Ultimately, quantitative analysis of every star, paying particular attention to the effects of rotational mixing and binarity, will be used to address fundamental questions in both stellar and cluster evolution.


2009 ◽  
Vol 702 (2) ◽  
pp. 940-954 ◽  
Author(s):  
N. Lehner ◽  
L. Staveley-Smith ◽  
J. C. Howk

2014 ◽  
Vol 790 (1) ◽  
pp. 24 ◽  
Author(s):  
Alex Drlica-Wagner ◽  
Germán A. Gómez-Vargas ◽  
John W. Hewitt ◽  
Tim Linden ◽  
Luigi Tibaldo

1994 ◽  
Vol 106 ◽  
pp. 632 ◽  
Author(s):  
Rebecca A. W. Elson ◽  
Duncan A. Forbes ◽  
Gerard F. Gilmore

Sign in / Sign up

Export Citation Format

Share Document