Large Magellanic Cloud bar: evidence of a warped bar

Subramaniam, Annapurni (2003) Large Magellanic Cloud bar: evidence of a warped bar The Astrophysical Journal Letters, 598 (1). L19-L22. ISSN 2041-8205

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Official URL: http://iopscience.iop.org/article/10.1086/380556?f...

Related URL: http://dx.doi.org/10.1086/380556

Abstract

The geometry of the LMC bar is studied using the dereddened mean magnitudes of the red clump stars (I0) from the Optical Gravitational Lensing Experiment II catalog. The value of I0 is found to vary in the east-west direction such that both the east and the west end of the bar are closer to us with respect to the center of the bar. The maximum observed variation has a statistical significance of more than 7.6 σ with respect to the maximum value of random error. The variation in I0 indicates the presence of warp in the bar of the LMC. The warp and the structures seen in the bar indicate that the bar could be a dynamically disturbed structure.

Item Type:Article
Source:Copyright of this article belongs to American Astronomical Society.
Keywords:Galaxies: Stellar Content; Galaxies: Structure; Magellanic Clouds
ID Code:106597
Deposited On:01 Feb 2018 12:04
Last Modified:01 Feb 2018 12:04

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