Excited-state hydroxyl maser catalogue from the methanol multibeam survey – I. Positions and variability

Author:

Avison A12,Quinn L J23,Fuller G A12,Caswell J L4,Green J A45,Breen S L4,Ellingsen S P6,Gray M D2,Pestalozzi M7,Thompson M A8,Voronkov M A4

Affiliation:

1. UK ALMA Regional Centre Node, Manchester, M13 9PL, UK

2. Jodrell Bank Centre for Astrophysics, Alan Turing Building, School of Physics and Astronomy, The University of Manchester, Manchester M13 9PL, UK

3. Bury College, Millennium Centre, Market Street, Bury BL9 0DB, UK

4. CSIRO Astronomy and Space Science, Australia Telescope National Facility, PO Box 76, Epping, NSW 2121, Australia

5. SKA Organization, Jodrell Bank Observatory, Lower Withington, Macclesfield, Cheshire SK11 9DL, UK

6. School of Physical Sciences, University of Tasmania, Private Bag 37, Hobart, TAS 7001, Australia

7. Istituto di Astrofisica e Planetologia Spaziali IAPS - INAF, via del Fosso del cavaliere 100, I-00133 Roma, Italy

8. Centre for Astrophysics Research, Science and Technology Research Institute, University of Hertfordshire, College Lane, Hatfield, Hertfordshire AL10 9AB, UK

Abstract

Abstract We present the results of the first complete unbaised survey of the Galactic plane for 6035-MHz excited-state hydroxyl (ex-OH) masers undertaken as part of the methanol multibeam (MMB) survey. These observations cover the Galactic longitude ranges 186° < l < 60° including the Galactic Centre. We report the detection of 127 ex-OH masers within the survey region, 47 being new sources. The positions of new detections were determined from interferometric observations with the Australia Telescope Compact Array. We discuss the association of 6035-MHz masers in our survey with the 6668-MHz masers from the MMB Survey, finding 37 likely CH3OH–ex-OH maser pairs with physical separations of ≤0.03 pc and 55 pairings separated by ≤0.1 pc. Using these we calculate for the first time an ex-OH maser lifetime of between 3.3 × 103 and 8.3 × 103 yr. We also discuss the variability of the 6035-MHz masers and detection rates of counterpart 6030-MHz ex-OH masers (28 per cent of our sample having detection at both frequencies).

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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