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Time-dependent numerical modelling of hydroxyl masers

Published online by Cambridge University Press:  16 July 2018

J. P. Maswanganye
Affiliation:
CSR, North-West University, Potchefstroom Campus, Private Bag X6001, Potchefstroom 2520 email: 24827142@nwu.ac.za
D. J. van der Walt
Affiliation:
CSR, North-West University, Potchefstroom Campus, Private Bag X6001, Potchefstroom 2520 email: 24827142@nwu.ac.za
S. Goedhart
Affiliation:
CSR, North-West University, Potchefstroom Campus, Private Bag X6001, Potchefstroom 2520 email: 24827142@nwu.ac.za SKA SA, 3rd Floor, The Park, Park Rd, Pinelands 7405, South Africa
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Abstract

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The statistical rate equations are used to model the OH masers to see if they will always have a one-to-one correspondence with the variation of dust temperature. It is concluded that one has to be careful to argue that the masers will always follow the dust temperature variation profile, and it is possible that different maser transitions from the same molecule respond differently to the same dust temperature variations.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2018 

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