A12COJ= 4→3 High-Velocity Cloud in the Large Magellanic Cloud

2005 ◽  
Vol 130 (4) ◽  
pp. 1635-1639 ◽  
Author(s):  
Sungeun Kim ◽  
Wilfred Walsh ◽  
Kecheng Xiao ◽  
Adair P. Lane
Keyword(s):  
High Velocity ◽  
Large Magellanic Cloud ◽  
Magellanic Cloud ◽  
Velocity Cloud ◽  
High Velocity Cloud

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 ◽  
...  
Keyword(s):  
High Velocity ◽  
Large Magellanic Cloud ◽  
Magellanic Cloud ◽  
Velocity Cloud ◽  
High Velocity Cloud ◽  
30 Doradus

scholarly journals Is High-Velocity Cloud Complex C Associated with the Galactic Warp?

2003 ◽  
Vol 20 (3) ◽  
pp. 263-269 ◽  
Author(s):  
Daisuke Kawata ◽  
Christopher Thom ◽  
Brad K. Gibson
Keyword(s):  
High Latitude ◽  
High Velocity ◽  
Large Magellanic Cloud ◽  
Alternative Interpretation ◽  
North Polar ◽  
Gas Cloud ◽  
Cloud Complex ◽  
Galactic Warp ◽  
Velocity Cloud ◽  
Spiral Arm

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.

PROPERTIES AND ORIGIN OF THE HIGH-VELOCITY GAS TOWARD THE LARGE MAGELLANIC CLOUD

2009 ◽  
Vol 702 (2) ◽  
pp. 940-954 ◽  
Author(s):  
N. Lehner ◽  
L. Staveley-Smith ◽  
J. C. Howk
Keyword(s):  
High Velocity ◽  
Large Magellanic Cloud ◽  
Magellanic Cloud

scholarly journals SEARCHING FOR DARK MATTER ANNIHILATION IN THE SMITH HIGH-VELOCITY CLOUD

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

scholarly journals DISCOVERY OF STAR FORMATION IN THE EXTREME OUTER GALAXY POSSIBLY INDUCED BY A HIGH-VELOCITY CLOUD IMPACT

2014 ◽  
Vol 795 (1) ◽  
pp. 66 ◽  
Author(s):  
Natsuko Izumi ◽  
Naoto Kobayashi ◽  
Chikako Yasui ◽  
Alan T. Tokunaga ◽  
Masao Saito ◽  
...  
Keyword(s):  
Star Formation ◽  
High Velocity ◽  
Velocity Cloud ◽  
High Velocity Cloud
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