2009/08/27 by Ye Xu, Y. Xu, M. A. Voronkov +7 · 3 citations
Chemistry · Physics and Astronomy · #Astronomical interferometer #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Chemistry #Interferometry #Maser #Merlin (protein) #Molecular Spectroscopy and Structure #Optics #Parallax #Physics #Proper motion #Star (game theory) #Star formation #Stars #Stellar, planetary, and galactic studies #Very-long-baseline interferometry #Wavelength #astro-ph.GA #astro-ph.SR
paper · pdf · doi:10.1051/0004-6361/200912135
A&A accepted 29 pages, 6 figures, 5 tables
arxiv created 2009/08/27 · openalex publication_date 2009/08/27 · arxiv updated 2015/05/14 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
The ATCA, MERLIN and VLA interferometers were used to measure the absolute positions of 35 6.7-GHz methanol masers to subarcsecond or higher accuracy. Our measurements represent essential preparatory data for Very Long Baseline Interferometry, which can provide accurate parallax and proper motion determinations of the star-forming regions harboring the masers. Our data also allow associations to be established with infrared sources at different wavelengths. Our findings support the view that the 6.7 GHz masers are associated with the earliest phases of high-mass star formation.