gion of the Local Group [@Kennicutt_Hodge_1986]. Figure \[HST\_LABOCA\] shows three-color compositions of the two regions N158 and N160 produced with images taken by the Wide Field Planetary Camera 2 (WFPC2) on board the Hubble Space Telescope (HST). Data are retrieved from the Hubble Legacy Archive (http://hla.stsci.edu/, Program IDs: 11807 and 8247 for N158 and N160 respectively). We overlay LABOCA 870 [$\mu$m]{} contours on both images for comparison between the spatial resolutions. The HST/WFPC2 observations of N158, N159 and N160 are discussed in details in @Fleener2010, @Heydari1999 and @Heydari2002 respectively.\
This H[ii]{} region (Fig. \[HST\_LABOCA\], left) possesses an elongated structure in the N-S direction. Two OB associations were first discovered in the region by @Lucke1970 who catalogued stellar associations across the whole LMC. One is associated with the southern part of N158, one with the north superbubble. Several studies have shown that this superbubble is dominated by a young stellar population of 2 to 6 Myr [@Testor1998; @Dunne2001].\
Observations of N159 in the K band by @Gatley1981 led to the discovery of the first extragalactic protostar. The stellar content of sub-structures of N159 was analysed in more detail by [@Deharveng1992] at optical wavelengths and @Meynadier2004 using JHK photometry. N159 presents characteristics of on-going star formation activity such as protostars, masers, young massive stars as well as High-Excitation Blobs (HEB), namely nebulae with turbulent media and strong stellar winds interacting with the ambient ionized gas. The Kuiper Airborne Observatory (KAO) has been used to probe the complex at far-infrared (FIR) wavelengths for the first time [@Werner1978; @Jones1986]. Later, @Jones2005 used [[*Spitzer*]{}]{}/IRAC observations to follow the protostars in N159 and constrain the nature of the upper end of the initial mass function (IMF) in the LMC.\
As in N159, massive star formation is well evolved in N160 (Fig. \[HST\_LABOCA\], right), with parent clouds 