Results 51 to 60 of about 423 (145)
Astrometry of the stellar image of U Her amplified by the circumstellar 22 GHz water masers
The 22 GHz H2O masers in the circumstellar envelope of the Mira variable star U Her have been observed with MERLIN using a phase referencing technique to determine accurate astrometric positions.
W. H. T. Vlemmings +5 more
core +1 more source
Variability of water masers in evolved stars on timescales of decades [PDF]
For several decades (1987-2015) we have been carrying out observations of water masers in the circumstellar envelopes (CSE's) of Mira variables, Red Supergiants (RSG's) and Semi-Regular Variables (SRV's) with the Medicina 32-m and Effelsberg 100-m ...
Winnberg, Anders +2 more
core +1 more source
CH3OH Thermal Lines Traces 6.7 GHz CH3OH Maser Variation of High-mass Protostar G353.273+0.641
This study reports an analysis of the 6.7 GHz CH _3 OH maser in the high-mass protostar G353.273+0.641 (G353), utilizing data from the Tianma Radio Telescope.
Shi-Min Song +3 more
doaj +1 more source
We present the results from long-term simultaneous monitoring observations of SiO and H _2 O masers toward the Mira variable star WX Serpentis. This study has been conducted with 21 m single-dish radio telescopes of the Korean VLBI Network from 2009 June
Jang-Ho Lim +6 more
doaj +1 more source
SiO masers in Mira variables at a single stellar phase
A hydrodynamic pulsation model for long-period M-type Mira variables is used to estimate the physical conditions of number density, temperature and velocity field in the circumstellar envelope of a model star of 1 M⊙, 332-d period, surface temperature ...
Humphreys, E. M L +11 more
core +3 more sources
SiO v = 1 J = 5 → 4 Maser Emission from the Root of the “Water Fountain” Source W 43A
We report here the first mapping of SiO v = 1 J = 5 → 4 maser emission toward the “water fountain” source W 43A in order to explore the central stellar system driving the collimated, bipolar, fast jet.
Hiroshi Imai +5 more
doaj +1 more source
Discovery of SiO masers in the Water Fountain source, IRAS 16552-3050 [Elektronisk resurs]
We report new detections of SiO ν = 1 and ν = 2 J = 1 → 0 masers in the water fountain source IRAS 16552-3050, which was observed with the Nobeyama 45 m telescope from March 2021 to April 2023.
Amada, Kei, +9 more
core +1 more source
Water and silicon-monoxide masers monitored towards the water fountain sources
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
Uscanga, L. +9 more
core +1 more source
Imaging the Jet of MWC 349A with Resolved Radio Recombination Line Emission from ALMA
Jets and disk winds arise from materials with excess angular momentum ejected from the accretion disks in forming stars. How these structures are launched and how they impact the gas within the innermost regions of these objects remains poorly understood.
Antonio Martínez-Henares +7 more
doaj +1 more source
First VLBI mapping of circumstellar
We report the first VLBI map of the $v=0$ $J=$ 1–0 maser line of 29SiO in the long-period variable star IRC +10011. We have found that this maser emission is composed of multiple spots distributed in an incomplete ring, suggesting that this maser is ...
J.-F. Desmurs +5 more
core +1 more source

