Maser Emission in G 339.884−1.259

We present multi–epoch VLBI observations of the methanol and water masers in the high–mass star formation region G 339.884−1.259, made using the Australian Long Baseline Array (LBA). Our sub–milliarcsecond precision measurements trace the proper motions of individual maser features in the plane of t...

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Veröffentlicht in:Proceedings of the International Astronomical Union 2017-09, Vol.13 (S336), p.334-335
Hauptverfasser: Krishnan, V., Moscadelli, L., Ellingsen, S. P., Bignall, H. E., Breen, S. L., Dodson, R., Hyland, L. J., Phillips, C. J., Reynolds, C., Stevens, J.
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Sprache:eng
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Zusammenfassung:We present multi–epoch VLBI observations of the methanol and water masers in the high–mass star formation region G 339.884−1.259, made using the Australian Long Baseline Array (LBA). Our sub–milliarcsecond precision measurements trace the proper motions of individual maser features in the plane of the sky. When combined with the direct line–of–sight radial velocity (vlsr), these measure the 3 D gas kinematics of the associated high–mass star formation region, allowing us to probe the dynamical processes to within 1000 AU of the core.
ISSN:1743-9213
1743-9221
DOI:10.1017/S1743921317010444