We have investigated the evolution of 12 water fountain sources in real time in the accompanying H2O 2o and SiO masers through our FLASHING (Finest Legacy Acquisitions of SiO-/ H2O 2o-maser Ignitions by Nobeyama Generation) project. It has been confirmed that these masers are excellent probes of new jet blob ejections, acceleration of the material supplied from the parental circumstellar envelope and entrained by the stellar jets yielding its deceleration. Possible periodic variations of the maser emission, reflecting properties of the central dying stars or binary systems, will be further investigated
We discovered new high-velocity components of H2O maser emission in one of the “water fountain” sour...
We report Very Long Baseline Array and Very Large Array observations of 22 GHz H2O and 43 GHz SiO (v...
Aims: The study of water masers at cosmological distances would allow us to investigate the parsec-s...
This is an Open Access article distributed under the terms of the Creative Commons Attribution Licen...
(Abridged) H2O masers in 14 SFRs have been monitored once every 2-3 months for up to 13 years. We in...
In this paper, we report new detections of SiO v = 1 and v = 2 J = 1 -> 0 masers in the "water fount...
We report the first detection of submillimeter water maser emission toward water-fountain nebulae, w...
We report the first detection of submillimeter water maser emission toward water-fountain nebulae, w...
We report Very Long Baseline Array and Very Large Array observations of 22 GHz H2O and 43 GHz SiO (v...
Water maser emission is a powerful tracer of the presence of embedded sources in dense clouds since ...
We present the results of the first detection of submillimeter water maser emission toward water-fou...
Abstract We performed an H2O maser survey towards 274 BGPS sources with 85 l < 193 ◦ using the Na...
We report Very Long Baseline Array and Very Large Array observations of 22 GHz H2O and 43 GHz SiO (v...
We present the results of simultaneous monitoring observations of H2O 6(1,6)-5(2,3) (22 GHz) and SiO...
The 25 years following the serendipitous discovery of megamasers have seen tremendous progress in th...
We discovered new high-velocity components of H2O maser emission in one of the “water fountain” sour...
We report Very Long Baseline Array and Very Large Array observations of 22 GHz H2O and 43 GHz SiO (v...
Aims: The study of water masers at cosmological distances would allow us to investigate the parsec-s...
This is an Open Access article distributed under the terms of the Creative Commons Attribution Licen...
(Abridged) H2O masers in 14 SFRs have been monitored once every 2-3 months for up to 13 years. We in...
In this paper, we report new detections of SiO v = 1 and v = 2 J = 1 -> 0 masers in the "water fount...
We report the first detection of submillimeter water maser emission toward water-fountain nebulae, w...
We report the first detection of submillimeter water maser emission toward water-fountain nebulae, w...
We report Very Long Baseline Array and Very Large Array observations of 22 GHz H2O and 43 GHz SiO (v...
Water maser emission is a powerful tracer of the presence of embedded sources in dense clouds since ...
We present the results of the first detection of submillimeter water maser emission toward water-fou...
Abstract We performed an H2O maser survey towards 274 BGPS sources with 85 l < 193 ◦ using the Na...
We report Very Long Baseline Array and Very Large Array observations of 22 GHz H2O and 43 GHz SiO (v...
We present the results of simultaneous monitoring observations of H2O 6(1,6)-5(2,3) (22 GHz) and SiO...
The 25 years following the serendipitous discovery of megamasers have seen tremendous progress in th...
We discovered new high-velocity components of H2O maser emission in one of the “water fountain” sour...
We report Very Long Baseline Array and Very Large Array observations of 22 GHz H2O and 43 GHz SiO (v...
Aims: The study of water masers at cosmological distances would allow us to investigate the parsec-s...