White, Glenn J. and Phillips, J. P.
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Observations of the J = 2→1 line of CO have been made towards 17 positions in the southern galactic plane where H2O masers have been detected. apparent self-absorption is found for RCW 38. In the vicinity of the Carina H2O maser the CO linewidth is broader than at neighbouring positions, which may be related to outflow. The J = 5→4 line of CS has been observed towards the H II region G 322.2+0.6. From a comparison with the J = 1→0 line observed previously, an H2 density of 8×105 cm-3 is derived.
|Item Type:||Journal Article|
|Copyright Holders:||1983 Royal Astronomical Society|
|Keywords:||carbon monoxide; molecular spectra; southern sky; star formation; HII regions; line spectra; nebulae; water masers|
|Academic Unit/School:||Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
|Interdisciplinary Research Centre:||Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)|
|Depositing User:||G. J. White|
|Date Deposited:||07 Jun 2012 09:25|
|Last Modified:||29 Nov 2016 22:45|
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