The stellar environment of SMC N81

Abstract

We present near infrared JHK imaging of the Small Magellanic Cloud compact H II region N81 using the ISAAC camera at the ESO Very Large Telescope (Antu). Our analysis of the stellar environment of this young massive star region reveals the presence of three new stellar populations in the surrounding field which are mainly composed of low mass stars. The main population is best fitted by evolutionary models for about 2 solar mass stars with an age of 1 Gyr. We argue that these populations are not physically associated with the H II region N81. Instead they are the result of a number of low mass star forming events through the depth of the SMC south of its Shapley's wing. The populations can rather easily be probed due to the low interstellar extinction in that direction.

11 pages, 5 figures, accepted for publication in A&A

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• $K$-band integral field spectroscopy and optical spectroscopy of massive young stellar objects in the Small Magellanic Cloud
• Stellar populations associated with the LMC Papillon Nebula
• Spitzer Mid-infrared Study of Compact HII Regions in the Magellanic Clouds
• INTEGRAL and XMM-Newton observations towards the unidentified MeV source GRO J1411-64