Results 31 to 40 of about 5,254,583 (200)
Time variations of water masers [PDF]
Symposium - International Astronomical Union, 2002 The strong water maser line at 22 GHz is an excellent tool for studying shocked and turbulent interstellar regions, especially, if simultaneous single-dish and VLBI data are available. After a brief review of 22 GHz time variation studies, we focus on effects caused by magnetic field pressure on observed properties of water masers.
Tarja Liljeström, Carl R. Gwinn
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An Investigation of Water Masers in High Mass Star Forming Regions [PDF]
, 2021 Within deep space are massive molecular clouds and within these molecular clouds, stars form. In these regions of star formation, masers can occur. I studied the presence of water masers within these high mass star forming regions. This was done in order
Webb, Eleanor A
core
Evolution of the outflow traced by water masers in the evolved star IRAS 18043 - 2116
, 2022 We present the spectral and spatial evolution of H2O masers associated with IRAS 18043-2116, a well-known water fountain hosting a high-velocity collimated jet, which has been found in the observations with the 45 m telescope of Nobeyama Radio ...
Amada, Kei, +7 more
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Water masers in dusty environments [PDF]
Astronomy & Astrophysics, 2004 14 pages, 10 figures; submitted to A& ...
Babkovskaia, Natalia, Poutanen, Juri
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A water maser flare in W49N [PDF]
Astronomy & Astrophysics, 2002 We report the results of our short time scale monitoring observations of W49N. Three water maser features were found to show obvious variations in flux density, line width and center velocity. Over a period of about 22 days, the -88.3, -56.9 and -12.8 km s(-1) features declined linearly in flux density at rates of 57, 113, 98.8 Jy per day, respectively.
J. J. Zhou, X. W. Zheng, Y. X. Chen
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A Search for Water Masers Toward YSO Candidates in the LMC [PDF]
, 2013 The proximity of the Large Magellanic Cloud (LMC) and its high star formation rate make it a prime candidate for the study of massive star formation outside of the Milky Way. A search for water masers associated with massive young stellar objects (YSOs)
Johanson, Adam, Migenes, Victor
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VLA observations of water masers towards 6.7 GHz methanol maser sources [PDF]
Astronomy & Astrophysics, 2010 accepted by Astronomy & ...
Bartkiewicz, A. +5 more
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Physical properties of Class I methanol masers [PDF]
, 2018 As first realised in the late 1980s, methanol masers come in two varieties, termed Class I and Class II. While Class II masers had observationally been extensively studied in the past, until recently relatively little attention was paid to Class I ...
Leurini, S. +3 more
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Type‐III Solar Radio Bursts at Mars: A 16.5‐Year Catalog From Mars Express‐MARSIS at 0.1–5.5 MHz
Space Weather, Volume 24, Issue 10, October 2026.Abstract The most intense radio feature in the Solar System are the solar Type‐III radio bursts, which are associated with electron beams that propagate along open magnetic field lines. Although solar radio bursts have been studied since the 1940s, observations remain mainly restricted within 1 AU.
Beatriz Sánchez‐Cano +22 more
wiley +1 more source
The Plant Journal, Volume 128, Issue 1, October 2026.SUMMARY Salt glands, developed in the epidermis of salt‐secreting mangrove plant Avicennia marina leaves and specialized in salt secretion, are critical for improving the survival under high saline habitats. However, the salt secretion mechanism in A. marina remains poorly understood. In this study, laser capture microdissection was employed to isolate
Ming‐Yue Wei +13 more
wiley +1 more source