ROTATION OF THE MILKY WAY AND THE FORMATION OF THE MAGELLANIC STREAM

Journal Article · Fri Dec 10 04:00:00 EST 2010 · Astrophysical Journal

DOI:https://doi.org/10.1088/0004-637X/725/1/369· OSTI ID:21474434

Ruzicka, Adam; Theis, Christian ^[1]; Palous, Jan ^[2]

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1. Institut fuer Astronomie der Universitaet Wien, Tuerkenschanzstrasse 17, A-1180 Wien (Austria)
2. Astronomical Institute of the Academy of Sciences of the Czech Republic, BocnI II 1401, 14131 Praha 4 (Czech Republic)

We studied the impact of the revisited values for the local standard of rest (LSR) circular velocity of the Milky Way on the formation of the Magellanic Stream. The LSR circular velocity was varied within its observational uncertainties as a free parameter of the interaction between the Large (LMC) and the Small Magellanic Clouds (SMC) and the Galaxy. We have shown that the large-scale morphology and kinematics of the Magellanic Stream may be reproduced as tidal features, assuming the recent values of the proper motions of the Magellanic Clouds. Automated exploration of the entire parameter space for the interaction was performed to identify all parameter combinations that allow for modeling the Magellanic Stream. Satisfactory models exist for the dynamical mass of the Milky Way within a wide range of 0.6 x 10{sup 12}-3.0 x 10{sup 12} M{sub sun} and over the entire 1{sigma} errors of the proper motions of the Clouds. However, the successful models share a common interaction scenario. The Magellanic Clouds are satellites of the Milky Way, and in all cases two close LMC-SMC encounters occurred within the last 4 Gyr at t < -2.5 Gyr and t {approx} -150 Myr, triggering the formation of the Stream and of the Magellanic Bridge, respectively. The latter encounter is encoded in the observed proper motions and inevitable in any model of the interaction. We conclude that the tidal origin of the Magellanic Stream implies the previously introduced LMC/SMC orbital history, unless the parameters of the interaction are revised substantially.

• OSTI ID: 21474434
• Journal Information: Astrophysical Journal, Journal Name: Astrophysical Journal Journal Issue: 1 Vol. 725; ISSN ASJOAB; ISSN 0004-637X
• Country of Publication: United States
• Language: English

Related Subjects

79 ASTRONOMY AND ASTROPHYSICS
EVOLUTION
GALACTIC EVOLUTION
GALAXIES
MAGELLANIC CLOUDS
MASS
MILKY WAY
MORPHOLOGY
MOTION
PROPER MOTION
ROTATION
SATELLITES
SIMULATION