Results 1 to 10 of about 7,116 (192)

VLA observations of water masers towards 6.7 GHz methanol maser sources [PDF]

open access: yesAstronomy & Astrophysics, 2010
22 GHz water and 6.7 GHz methanol masers are usually thought as signposts of early stages of high-mass star formation but little is known about their associations and the physical environments they occur in. The aim was to obtain accurate positions and
A. Bartkiewicz   +43 more
core   +2 more sources

Water Masers in the Andromeda Galaxy: I. A Survey for Water Masers, Ammonia, and Hydrogen Recombination Lines [PDF]

open access: yesThe Astrophysical Journal, 2016
We report the results of a Green Bank Telescope survey for water masers, ammonia (1,1) and (2,2), and the H66-alpha recombination line toward 506 luminous compact 24 micron-emitting regions in the Andromeda Galaxy (M31).
Amiri, Nikta   +3 more
core   +2 more sources

The Parallax and 3D Kinematics of Water Masers in the Massive Star-forming Region G034.43+0.24

open access: yesThe Astrophysical Journal, 2023
We report a measurement of the trigonometric parallax of 22 GHz water masers in the massive star-forming region G034.43+0.24 as part of the Bar and Spiral Structure Legacy Survey using the Very Long Baseline Array.
Xiaofeng Mai   +14 more
doaj   +1 more source

Unusually Powerful Flare Phenomenon of the Water Maser in W51 and the Possibility of Detecting Gravitational Radiation from It

open access: yesThe Astrophysical Journal, 2023
Because of detailed monitoring of the 22.2 GHz water maser, carried out from 2021 October to 2023 May, a very powerful flare phenomenon was detected in the galactic object W51 near the radial velocity of 60 km s ^−1 with the amplitude of 140 kJy.
A. E. Volvach   +2 more
doaj   +1 more source

Physical Environments of the Luminosity Outburst Source NGC 6334I Traced by Thermal and Maser Lines of Multiple Molecules

open access: yesThe Astrophysical Journal Supplement Series, 2023
We have conducted a systematic line survey, primarily focused on transitions of the methanol and ammonia molecules, and monitoring observations of masers toward the high-mass star-forming region NGC 6334I.
Jiong-Heng Wu   +12 more
doaj   +1 more source

Simultaneous Time-monitoring Observations of H2O and SiO Masers toward the Supergiant VX Sagittarii

open access: yesThe Astrophysical Journal Supplement Series, 2023
We performed simultaneous monitoring observations of the 22.2 GHz H _2 O and 43.1/42.8/86.2/129.3 GHz SiO masers toward the red supergiant VX Sagittarii using the Korean VLBI Network single-dish telescopes.
Dong-Hwan Yoon   +4 more
doaj   +1 more source

Water maser emission in IC 342 [PDF]

open access: yesAstronomy & Astrophysics, 2002
The detection of 22 GHz water vapor emission from IC342 is reported, raising the detection rate among northern galaxies with 100 micron IRAS point source fluxes > 50 Jy to 16%. The maser, associated with a star forming region 10-15 arcsec west of the nucleus, consists of a single 0.5 km/s wide feature and reaches an isotropic luminosity of 0.01 ...
Tarchi A.   +3 more
openaire   +3 more sources

183 GHz Water Megamasers in Active Galactic Nuclei: A New Accretion Disk Tracer

open access: yesThe Astrophysical Journal, 2023
We present the results of an Atacama Large Millimeter/submillimeter Array survey to identify 183 GHz H _2 O maser emission from active galactic nuclei (AGNs) already known to host 22 GHz megamaser systems.
Dominic W. Pesce   +5 more
doaj   +1 more source

Evolution of the Outflow in the Water Fountain Source IRAS 18043–2116

open access: yesThe Astrophysical Journal, 2023
We present the spectral and spatial evolution of H _2 O masers associated with the water fountain source IRAS 18043−2116, found in observations with the Nobeyama 45 m Telescope and the Australia Telescope Compact Array. We have found new highest-velocity
L. Uscanga   +7 more
doaj   +1 more source

Proper Motions of Water Masers in W49 N Measured by KaVA

open access: yesThe Astrophysical Journal, 2023
We report the proper motions of 22 GHz water masers toward W49 N that were observed by the KVN and VERA Array (KaVA) during 2017 February–May. We found 263, 268, and 310 features in three successive epochs; they were distributed in a region of size 4 × 4
Kitiyanee Asanok   +8 more
doaj   +1 more source

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