Add to ORKGWe report on astrometric observations of H2O masers around the red supergiant VY Canis Majoris carried out with VLBI Exploration of Radio Astrometry (VERA). Based on astrometric monitoring for 13 months, we successfully measured a trigonometric parallax of 0.88˙0.08 mas, corresponding to a distance of 1.14+0:110:09 kpc. Thi
We report on the measurement of the trigonometric parallaxes of 1612 MHz hydroxyl masers around two ...
The most powerful tool for measuring distances within our Galaxy is the annual parallax. We carried ...
Precise structure and dynamics of the Milky Way Galaxy are still relatively ambiguous due to difficu...
We report on results of multi-epoch VLBI observations of H2O masers associated with a low-mass young...
Using the VLBI Exploration of Radio Astrometry (VERA), we measured the trigonometric parallax of an ...
Abstract We report astrometric results of VLBI phase-referencing observations of 22 GHz H2O masers e...
We have used the Japanese VLBI array VERA to perform high-precision astrometry of an H2O maser sourc...
We report astrometric results of phase-referencing very long baseline interferometry observations of...
We performed the astrometry of H2O masers in the Galactic star-forming region Onsala 2 North (ON 2 ...
Abstract We report a trigonometric parallax measurement of 22 GHz H2O masers toward the semi-regular...
We performed the astrometry of H2O masers in the Galactic star-forming region Onsala 2 North (ON 2 N...
We report on 43 GHz v=1, J=1-0 SiO maser proper motions in the circurnstellar envelope of the M-type...
We report on results of astrometric observations of H2O masers in the "water fountain" source IRAS 1...
We present the very long baseline interferometry H2O maser monitoring observations of the red superg...
International audienceIRAS 16293-2422 is a very well-studied young stellar system seen in projection...
We report on the measurement of the trigonometric parallaxes of 1612 MHz hydroxyl masers around two ...
The most powerful tool for measuring distances within our Galaxy is the annual parallax. We carried ...
Precise structure and dynamics of the Milky Way Galaxy are still relatively ambiguous due to difficu...
We report on results of multi-epoch VLBI observations of H2O masers associated with a low-mass young...
Using the VLBI Exploration of Radio Astrometry (VERA), we measured the trigonometric parallax of an ...
Abstract We report astrometric results of VLBI phase-referencing observations of 22 GHz H2O masers e...
We have used the Japanese VLBI array VERA to perform high-precision astrometry of an H2O maser sourc...
We report astrometric results of phase-referencing very long baseline interferometry observations of...
We performed the astrometry of H2O masers in the Galactic star-forming region Onsala 2 North (ON 2 ...
Abstract We report a trigonometric parallax measurement of 22 GHz H2O masers toward the semi-regular...
We performed the astrometry of H2O masers in the Galactic star-forming region Onsala 2 North (ON 2 N...
We report on 43 GHz v=1, J=1-0 SiO maser proper motions in the circurnstellar envelope of the M-type...
We report on results of astrometric observations of H2O masers in the "water fountain" source IRAS 1...
We present the very long baseline interferometry H2O maser monitoring observations of the red superg...
International audienceIRAS 16293-2422 is a very well-studied young stellar system seen in projection...
We report on the measurement of the trigonometric parallaxes of 1612 MHz hydroxyl masers around two ...
The most powerful tool for measuring distances within our Galaxy is the annual parallax. We carried ...
Precise structure and dynamics of the Milky Way Galaxy are still relatively ambiguous due to difficu...