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IRAS 12063-6259
IRAS 12063-6259 is a compact H II region which lies at a heliocentric distance of roughly 9.5 kpc and a galactocentric distance of 9.3 kpc.〔Caswell, J.L., & Haynes, R.F. 1987, A&A, 171, 261〕 Although previously classified as a planetary nebula as well as an H II region, this source is now solely classified as a normal compact H II region, due to its colour criteria,〔Wood, D.O.S., & Churchwell, E. 1989, ApJ, 340, 265〕 it infrared luminosity, and its spectral content.〔Peeters, E., Martín-Hernández, N.L., Damour, F., Cox, P., Roelfsema, P.R., Balutea, J.-P., Tielens, A.G.G.M., Churchwell, E., Kessler, M.F., Mathis, J.S., Morisset, C., & Schaerer, D. 2002, A&A, 381, 571〕
Radio observations from the Australia Telescope Compact Array (ATCA) reveal IRAS 12063-6259 to consist of a compact object roughly 16"x7" which is embedded in a low brightness region 28"x25". The compact region contains two compact objects at 4.8 GHz, labelled Radio A and Radio B, while at higher frequencies (8.6 GHz) Radio B is further resolved into subcomponents B1 and B2. This complex substructure points towards the presence of multiple ionising stars rather than a single star.〔Martín-Hernández, N.L., van der Hulst, J.M., & Tielens, A.G.G.M. 2003, A&A, 407, 957〕
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