Description of source "20081+3122" from Kim et al. (2015)


Kurtz et al. (1994) detected an unresolved UCHII to-ward this object using the Very Large Array (VLA).

Xu et al. (2006) mapped this source in the CO J=1 0 line using the Nobeyama Radio Observatory (NRO) 45 m telescope (FWHM=15") and detected a bipolar outow. Kumar et al. (2004) also mapped this object in the CO J=21 and SiO J=21 lines at signicantly higher angular resolutions using the IRAM Plateau de Bure Interferometer (PdBI) and claimed to detect four bipolar outows. The authors cautioned, however, that their maps do not reveal most of the large-scale struc-tures in this region and that the CO data quality was not good because of poor weather condition. This source was for the rst time mapped in the CO J=21 line using a single-dish telescope in this study.