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- W3105979291 abstract "In this paper we present Combined Array for Research in Millimeter-wave Astronomy (CARMA) 3.5 mm observations and SubMillimeter Array (SMA) 870 microns observations toward the high-mass star-forming region IRAS 1816-2048, the core of the HH 80/81/80N system. Molecular emission from HCN, HCO+ and SiO is tracing two molecular outflows (the so-called Northeast and Northwest outflows). These outflows have their origin in a region close to the position of MM2, a millimeter source known to harbor a couple protostars. We estimate for the first time the physical characteristics of these molecular outflows, which are similar to those of 1000-5000 Lo protostars, suggesting that MM2 harbors high-mass protostars. High-angular resolution CO observations show an additional outflow due southeast. We identify for the first time its driving source, MM2(E), and see evidence of precession. All three outflows have a monopolar appearance, but we link the NW and SE lobes, explaining their asymmetric shape as a consequence of possible deflection." @default.
- W3105979291 created "2020-11-23" @default.
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- W3105979291 date "2013-11-06" @default.
- W3105979291 modified "2023-10-16" @default.
- W3105979291 title "MULTIPLE MONOPOLAR OUTFLOWS DRIVEN BY MASSIVE PROTOSTARS IN IRAS 18162-2048" @default.
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- W3105979291 doi "https://doi.org/10.1088/0004-637x/778/1/72" @default.
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