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• W3104193732 abstract "Aims. We carried out sub-arcsecond resolution observations towards the high-mass star formation region G 19.61−0.23, in both continuum and molecular line emission. While the centimeter continuum images, representing ultra compact HII regions, will be discussed in detail in a forthcoming paper, here we focus on the (sub)mm emission, devoting special attention to the hot molecular core (HMC)." @default.
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• W3104193732 date "2010-12-02" @default.
• W3104193732 modified "2023-09-27" @default.
• W3104193732 title "Infall, outflow, and rotation in the G19.61-0.23 hot molecular core" @default.
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• W3104193732 doi "https://doi.org/10.1051/0004-6361/201014402" @default.
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