Mapping Observations of 6.7 GHz Methanol Masers with Japanese VLBI Network
arXiv:0710.4872 · doi:10.1093/pasj/60.1.23
Abstract
We have observed 13 methanol maser sources associated with massive star-forming regions; W3(OH), Mon R2, S 255, W 33A, IRAS 18151-1208, G 24.78+0.08, G 29.95-0.02, IRAS 18556+0136, W 48, OH 43.8-0.1, ON 1, Cep A and NGC 7538 at 6.7 GHz using the Japanese VLBI Network (JVN). Twelve of the thirteen sources were detected at our longest baseline of 50 M, and their images are presented. Seven of them are the first VLBI images at 6.7 GHz. This high detection rate and the small fringe spacing of 4 milli-arcsecond suggest that most of the methanol maser sources have compact structure. Given this compactness as well as the known properties of long-life and small internal-motion, this methanol maser line is suitable for astrometry with VLBI.
15 pages, 13 figures, accepted for publication in PASJ
References in corpus (9)
- The Distance to the Perseus Spiral Arm in the Milky Way
- A general catalogue of 6.7 GHz methanol masers. I: data
- Water maser motions in W3(OH) and a determination of its distance
- Methanol masers : Reliable tracers of the early stages of high-mass star formation
- The Arecibo Methanol Maser Galactic Plane Survey--I: Data
- Methanol Maser Polarization in W3(OH)
- Ring shaped 6.7 GHz methanol maser emission around a young high-mass star
- Associations of water and methanol masers at milli-arcsec angular resolution in two high-mass young stellar objects
- The structure of Onsala 1 star forming region
Cited by in corpus (23)
- A necklace of dense cores in the high-mass star forming region G35.20-0.74N: ALMA observations
- A wide-angle outflow with the simultaneous presence of a high-velocity jet in the high-mass Cepheus A HW2 system
- Observations of 6.7 GHz Methanol Masers with EAVN I: VLBI Images of the first Epoch of Observations
- The Spatial Distribution of Organics toward the High-Mass YSO NGC 7538 IRS9
- Planar infall of CH3OH gas around Cepheus A HW2
- EVN observations of 6.7 GHz methanol maser polarization in massive star-forming regions
- KFPA Examinations of Young STellar Object Natal Environments (KEYSTONE): Hierarchical Ammonia Structures in Galactic Giant Molecular Clouds
- Rotating and infalling motion around the high-mass young stellar object Cepheus A-HW2 observed with the methanol maser at 6.7 GHz
- Dynamics of the 6.7 and 12.2 GHz methanol masers around Cepheus A HW2
- The First Very Long Baseline Interferometry Image of 44 GHz Methanol Maser with the KVN and VERA Array (KaVA)
- ALMA Observations of the IRDC Clump G34.43+00.24 MM3: 278 GHz Class I Methanol Masers
- A Synchronized Variation of the 6.7 GHz Methanol Maser in Cepheus A
- EVN observations of 6.7 GHz methanol masers in clusters of massive young stellar objects
- 6.7GHz methanol maser variability in Cepheus A
- Magnetic field regulated infall on the disc around the massive protostar Cepheus A HW2
- Bursting Activity in a High-Mass Star-Forming Region G33.64-0.21 Observed with the 6.7 GHz Methanol Maser
- New evidence for Dicke's superradiance in the 6.7 GHz methanol spectral line in the interstellar medium
- EVN observations of 6.7 GHz methanol maser polarization in massive star-forming regions IV. Magnetic field strength limits and structure for 7 additional sources
- Internal Motion of 6.7-GHz Methanol Masers in H II Region S269
- Maser Flares Driven by Variations in Pumping and Background Radiation
- Distribution and excitation of thermal methanol in 6.7 GHz maser bearing star-forming regions; I. The nearby source Cepheus A
- Masers in star forming regions
- Physical conditions around high-mass young star-forming objects via simultaneous observations of excited OH and methanol masers