# The VMC Survey - XXIV. Signatures of tidally stripped stellar populations from the inner Small Magellanic Cloud

@article{Subramanian2017TheVS,
title={The VMC Survey - XXIV. Signatures of tidally stripped stellar populations from the inner Small Magellanic Cloud},
author={Smitha Subramanian and Stefano Rubele and Ning-Chen Sun and L{\'e}o Girardi and Richard de Grijs and Jacco Th. van Loon and Maria-Rosa L. Cioni and Andr{\'e}s E. Piatti and Kenji Bekki and James P. Emerson and Valentin D. Ivanov and Leandro de O Kerber and Marcella Marconi and Vincenzo Ripepi and Benjamin L. Tatton},
journal={Monthly Notices of the Royal Astronomical Society},
year={2017},
volume={467},
pages={2980-2995}
}
• Published 20 January 2017
• Physics
• Monthly Notices of the Royal Astronomical Society
We study the luminosity function of intermediate-age red-clump stars using deep, near-infrared photometric data covering $\sim$ 20 deg$^2$ located throughout the central part of the Small Magellanic Cloud (SMC), comprising the main body and the galaxy's eastern wing, based on observations obtained with the VISTA Survey of the Magellanic Clouds (VMC). We identified regions which show a foreground population ($\sim$11.8 $\pm$ 2.0 kpc in front of the main body) in the form of a distance bimodality…

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## References

SHOWING 1-10 OF 34 REFERENCES

### A TIDALLY STRIPPED STELLAR COMPONENT OF THE MAGELLANIC BRIDGE

• Physics, Geology
• 2013
Deep photometry of the Small Magellanic Cloud (SMC) stellar periphery (R = 4°, 4.2 kpc) is used to study its line-of-sight depth with red clump (RC) stars. The RC luminosity function is affected

### THE MAGELLANIC INTER-CLOUD PROJECT (MAGIC). I. EVIDENCE FOR INTERMEDIATE-AGE STELLAR POPULATIONS IN BETWEEN THE MAGELLANIC CLOUDS

• Physics
• 2013
The origin of the gas in between the Magellanic Clouds (MCs)—known as the “Magellanic Bridge” (MB)—is puzzling. Numerical simulations suggest that the MB formed from tidally stripped gas and stars in

### The VMC survey - XIV. First results on the look-back time star formation rate tomography of the Small Magellanic Cloud

• Physics
• 2015
We analyse deep images from the VISTA survey of the Magellanic Clouds in the YJKs filters, covering 14 sqrdeg (10 tiles), split into 120 subregions, and comprising the main body and Wing of the Small

### The VMC survey – XV. The Small Magellanic Cloud–Bridge connection history as traced by their star cluster populations

• Physics
• 2015
We present results based on YJKs photometry of star clusters located in the outermost, eastern region of the Small Magellanic Cloud (SMC). We analysed a total of 51 catalogued clusters whose

### OGLE-ING THE MAGELLANIC SYSTEM: STELLAR POPULATIONS IN THE MAGELLANIC BRIDGE

• Physics
• 2014
We report the discovery of a young stellar bridge that forms a continuous connection between the Magellanic Clouds. This finding is based on number density maps for stellar populations found in data

### The Magellanic Bridge: The Nearest Purely Tidal Stellar Population

We report on observations of the stellar populations in 12 fields spanning the region between the Magellanic Clouds, made with the Mosaic II camera on the 4 m telescope at the Cerro-Tololo

### The MAGellanic Inter-Cloud (MAGIC) project – II. Slicing up the Bridge

• Physics
• 2015
The origin of the gas in between the Magellanic Clouds (MCs), known as the Magellanic Bridge, has always been the subject of controversy. To shed light into this, we present the results from the

### The origin of the microlensing events observed towards the LMC and the stellar counterpart of the Magellanic stream

• Physics, Geology
• 2013
We introduce a novel theoretical model to explain the long-standing puzzle of the nature of the microlensing events reported towards the Large Magellanic Cloud (LMC) by the MACHO and OGLE

### THE THREE-DIMENSIONAL STRUCTURE OF THE SMALL MAGELLANIC CLOUD

• Physics
• 2012
The three-dimensional structure of the inner Small Magellanic Cloud (SMC) is investigated using the red clump (RC) stars and the RR Lyrae stars (RRLS), which represent the intermediate-age and the

### The Magellanic Stream, High-Velocity Clouds, and the Sculptor Group

• Physics
• 2003
The Magellanic Stream is a 100° × 10° filament of gas that lies within the Galactic halo and contains ~2 × 108 M☉ of neutral hydrogen. In this paper we present data from the H I Parkes All Sky Survey