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<https://discovery.ucl.ac.uk/id/eprint/10192694> <http://purl.org/dc/terms/title> "Star formation signatures in the condensation  downstream of HH80N"^^<http://www.w3.org/2001/XMLSchema#string> .
<https://discovery.ucl.ac.uk/id/eprint/10192694> <http://purl.org/ontology/bibo/abstract> "HH80N is one of the Herbig-Haro objects that have associated quiescent dense\r\nclumps. We report CO and CS BIMA observations that reveal star formation within\r\nthe HH80N dense clump. The CO emission reveals clearly a bipolar molecular\r\noutflow centered on the dense clump. The CS emission traces a ring-like\r\nstructure of radius ~0.24 pc. The CS kinematics shows that the ring is\r\ncollapsing with an infall speed of ~0.6 km/s. The required mass to produce the\r\ncollapse is in agreement with previous ammonia observations of the 20 solar\r\nmass core, which is embedded within the CS structure. However, we cannot\r\ndiscard that the ring structure is expanding driven by protostellar winds, if\r\nthe CS abundance if unusually high and the CO momentum rate is much higher than\r\nthat measured, due to inclination and optical depth effects. The properties of\r\nthe molecular outflow and of the dense core suggest that it harbors a Class 0\r\nobject. There are also signatures of interaction of the HH 80/81/80N outflow\r\nwith the dense gas. In particular it is possible that the HH 80/81/80N outflow\r\nhas triggered or at least speed up the star formation in this region."^^<http://www.w3.org/2001/XMLSchema#string> .
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