Hindson, L.; Thommpson, M. A.; Urquhart, J. S.; Clark, J. S. and Davies, B.
Due to copyright restrictions, this file is not available for public download
Click here to request a copy from the OU Author.
|DOI (Digital Object Identifier) Link:||http://doi.org/10.1111/j.1365-2966.2010.17154.x|
|Google Scholar:||Look up in Google Scholar|
We present wide-area radio (12 mm) Mopra telescope observations of the complex and rich massive star-forming region G305. Our goals are to determine the reservoir for star formation within G305 using NH3 to trace the dense molecular content, and thus the gas available to form stars; estimate physical parameters of detected NH3 clumps (temperature, column density, mass, etc.); locate current areas of active star formation via the presence of H2O and methanol masers and the distribution of young stellar objects (YSOs) and ultra-compact HII regions associated with this region. This paper details the NH3 (J, K), (1,1), (2,2) and (3,3) inversion transition and 22 GHzH2O maser observations.We observed a~1°.5×1° region with ~2 arcmin angular resolution and a sensitivity of ~60 mK per 0.4 km s?1 channel.We identify 15 NH3 (1,1), 12 NH3 (2,2) and 6 NH3 (3,3) clumps surrounding the central HII region. The sizes of the clumps vary between <2.6 and 10.1 pc; the average kinetic temperature of the gas is 25 K. We calculate clump masses of >104M¤ and find the total molecular mass of the complex to be ~6×105M¤.We note the positions of 56 star formation tracers, and discover a high degree of correlation with detected NH3 clumps.We have detected 16 H2O masers and find they correlate with the detected ammonia clumps. In general, they are found closer to the NH3 clump cores than star formation tracers of later evolutionary stages.
|Item Type:||Journal Article|
|Copyright Holders:||2010 The Authors, 2010 RAS (Journal compilation)|
|Extra Information:||N.B. Due to technical limitations not all the symbols in the abstract have been faithfully reproduced.|
|Keywords:||masers; stars: formation; ISM: clouds; ISM: molecules; radio lines: ISM|
|Academic Unit/Department:||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:||J. Simon Clark|
|Date Deposited:||27 Oct 2010 12:01|
|Last Modified:||05 Oct 2016 01:46|
|Share this page:|