MAGMO: Polarimetry of 1720-MHz OH Masers towards Southern Star Forming Regions
arXiv:2001.06180 · doi:10.1093/mnras/staa167
Abstract
From targeted observations of ground-state OH masers towards 702 Multibeam (MMB) survey 6.7-GHz methanol masers, between Galactic longitudes 186 through the Galactic centre to 20, made as part of the `MAGMO' project, we present the physical and polarisation properties of the 1720-MHz OH maser transition, including the identification of Zeeman pairs. We present 10 new and 23 previously catalogued 1720-MHz OH maser sources detected towards star formation regions. In addition, we also detected 16 1720-MHz OH masers associated with supernova remnants and two sites of diffuse OH emission. Towards the 33 star formation masers, we identify 44 Zeeman pairs, implying magnetic field strengths ranging from 11.4 to 13.2 mG, and a median magnetic field strength of 6 mG. With limited statistics, we present the in-situ magnetic field orientation of the masers and the Galactic magnetic field distribution revealed by the 1720-MHz transition. We also examine the association statistics of 1720-MHz OH SFR masers with other ground-state OH masers, excited-state OH masers, class I and class II methanol masers and water masers, and compare maser positions with mid-infrared images of the parent star forming regions. Of the 33 1720-MHz star formation masers, ten are offset from their central exciting sources, and appear to be associated with outflow activity.
References in corpus (15)
- A Catalog of Extended Green Objects (EGOs) in the GLIMPSE Survey: A new sample of massive young stellar object outflow candidates
- Rotation Measures of Extragalactic Sources Behind the Southern Galactic Plane: New Insights into the Large-Scale Magnetic Field of the Inner Milky Way
- Placing Confidence Limits on Polarization Measurements
- The 6-GHz Multibeam Maser Survey I. Techniques
- Trigonometric parallaxes of star forming regions in the Sagittarius spiral arm
- The RMS Survey: Mid-Infrared Observations of Candidate Massive YSOs in the Southern Hemisphere
- Accurate water maser positions from HOPS
- Polarization measurements analysis I. Impact of the full covariance matrix on polarization fraction and angle measurements
- A String of Radio Emission Associated with IRAS 16562-3959: A Collimated Jet Emanating from a Luminous Massive YSO
- The almost ubiquitous association of 6.7 GHz methanol masers with dust
- First Parallax Measurements Towards a 6.7 GHz Methanol Maser with the Australian Long Baseline Array - Distance to G339.884-1.259
- S-PASS/ATCA: a window on the magnetic universe in the southern hemisphere
- MALT-45: A 7 mm survey of the southern Galaxy - I. Techniques and spectral line data
- A search for water masers associated with class II methanol masers - I. Longitude range 6 to 20 degrees
- MALT-45: A 7mm survey of the southern Galaxy - II. ATCA follow-up observations of 44GHz class I methanol masers
Cited by in corpus (5)
- Turbulent dynamo in the two-phase interstellar medium
- SPLASH: The Southern Parkes Large-Area Survey in Hydroxyl -- Data Description & Release
- A Comparison of Multi-Phase Magnetic Field Tracers in a High-Galactic Latitude Region of the Filamentary Interstellar Medium
- GNOMES II: Analysis of the Galactic diffuse molecular ISM in all four ground state hydroxyl transitions using Amoeba
- HI filaments as potential compass needles? Comparing the magnetic field structure of the Small Magellanic Cloud to the orientation of GASKAP-HI filaments