Results 71 to 80 of about 176 (166)
Time variability of astrophysical masers [PDF]
M. Salem, M. S. Middleton
openaire +1 more source
Bar-driven Shocks in NGC 1365 Revealed by the Most Luminous Extragalactic Class I Methanol Maser
We report the first detection of the 36.2 GHz (4 _−1 → 3 _0 E) Class I methanol (CH _3 OH) maser in the central region of the barred spiral galaxy NGC 1365.
Xi Chen +7 more
doaj +1 more source
Extragalactic Class I methanol masers are well-established tracers of bar-driven shocks in several nearby galaxies, but whether active galactic nucleus (AGN)-driven outflows can also excite such masers has remained unclear.
Xi Chen +6 more
doaj +1 more source
Survey of S-type AGB Stars Using the KVN Four-band Receiving System: SMASTES II
We present the observational results of Simultaneous Multi-mAser Survey Toward Evolved Stars (SMASTES) II for 150 S-type asymptotic giant branch stars. Observations have been performed from 2023 September to 2024 March using the upgraded wide four-band ...
Seong-Min Son +5 more
doaj +1 more source
Radio Astronomical Antennas in the Central African Region to Improve the Sampling Function of the VLBI Network in the SKA Era? [PDF]
Atemkeng M +4 more
europepmc +1 more source
We present multiepoch, multiband Atacama Large Millimeter/submillimeter Array imaging of the new Class II millimeter methanol masers excited during the accretion outburst of the massive protostar G358.93−0.03 MM1. The highest angular resolution image (24
T. R. Hunter +5 more
doaj +1 more source
From 2019 January to June, the high-mass young stellar object G358.93-0.03 underwent a remarkable accretion burst. Detecting variations in the physical and kinematic environments during episodic accretion is essential for exploring such events. Searching
Shi-jie Zhang +5 more
doaj +1 more source
Field and intensity correlations: the Siegert relation from stars to quantum emitters. [PDF]
Lassègues P +11 more
europepmc +1 more source
Maser Radiation in an Astrophysical Context (Overview)
In this paper we will look at the phenomenon of Microwave Amplification by Stimulated Emission of Radiation (a maser system). We begin by deriving amplification by stimulated emission using time-dependent perturbation theory, in which the perturbation provided by external radiation.
openaire +2 more sources
Survey of Oxygen-rich AGB Stars Using the KVN 4 Receiving Bands—SMASTES. I.
Simultaneous observations of 19 H _2 O and SiO maser and thermal lines were performed toward 155 M-type oxygen-rich (O-rich) AGB stars. We used the upgraded four-band (22/43/86/129 GHz) wide receiving system of the Korean VLBI Network (KVN).
Hyeon Baek +5 more
doaj +1 more source

