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- W3036699304 abstract "IRAS 12272-6240 is a complex star forming region with a compact massive dense clump and several associated masers, located at a well-determined distance of $d=9.3$ kpc from the Sun. For this study, we obtained sub-arcsec broad- and narrow-band near-IR imaging and low-resolution spectroscopy with the Baade/Magellan telescope and its camera PANIC. Mosaics of size $2 times 2$ square arcmin in the $JHK_s$ bands and with narrow-band filters centred in the 2.12 $mu$m H$_2$ and 2.17 $mu$m Br$gamma$ lines were analysed in combination with HI-GAL/{sl Herschel} and archive IRAC/{sl Spitzer} and {sl WISE} observations. We found that the compact dense clump houses two Class~I YSOs that probably form a 21 kAU-wide binary system. Its combined 1 to 1200 $mu$m SED is consistent with an O9V central star with a $10^{-2} M_odot$ disc and a $1.3 times 10^4 M_odot$ dust envelope. Its total luminosity is $8.5 times 10^4 L_odot$. A series of shocked H$_2$ emission knots are found in its close vicinity, confirming the presence of outflows. IRAS 12272-6240 is at the centre of an embedded cluster with a mean age of 1 Myr and 2.6 pc in size that contains more than 150 stars. At its nucleus, we found a more compact and considerably younger sub-cluster containing the YSOs. We also identified and classified the O-type central stars of two dusty radio/IR HII regions flanking the protostars. Our results confirm that these elements form a single giant young complex where massive star formation processes started some 1 million years ago and is still active." @default.
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- W3036699304 date "2020-06-20" @default.
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- W3036699304 title "An infrared study of the high-mass, multistage star-forming region IRAS 12272−6240" @default.
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- W3036699304 doi "https://doi.org/10.1093/mnras/staa1772" @default.
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