Results 111 to 120 of about 4,740 (197)
Field and intensity correlations: the Siegert relation from stars to quantum emitters. [PDF]
Lassègues P +11 more
europepmc +1 more source
The possibility of using astrophysical observations of rotational transitions in the methanol molecule to measure, or constrain temporal and spatial variations in the proton-to-electron mass ratio (mu) has recently been investigated by several groups ...
Breen, Shari +2 more
core +1 more source
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
A database of circumstellar OH masers
We present a new database of circumstellar OH masers at 1612, 1665, and 1667 MHz in the Milky Way galaxy. The database (version 2.4) contains 13655 observations and 2341 different stars detected in at least one transition.
Bunzel, F., Engels, D.
core +1 more source
Cumulene carbenes in TMC-1: Astronomical discovery of <i>l</i>-H<sub>2</sub>C<sub>5</sub> <sup>★</sup>. [PDF]
Cabezas C +6 more
europepmc +1 more source
We present high angular resolution Submillimeter Array (SMA) and Karl G. Jansky Very Large Array (VLA) observations of the massive protocluster G18.67+0.03.
Brogan, C. L. +6 more
core +1 more source
Time variability of astrophysical masers [PDF]
M. Salem, M. S. Middleton
openaire +1 more source
Mechanisms for the circular polarization of astrophysical OH masers in star-forming regions and the inferred magnetic fields [PDF]
Results of further calculations to explore the cause for the circular polarization of astrophysical OH masers in regions of star formation are presented.
Deguchi, Shuji, Watson, William D.
core +1 more source
Main-sequence radio pulse emitters (MRPs) are magnetic early-type stars that produce coherent radio emission observed in the form of periodic radio pulses. The emission mechanism behind this is the electron-cyclotron maser emission (ECME).
Barnali Das +2 more
doaj +1 more source
Cloud-cloud collision as drivers of the chemical complexity in Galactic Centre molecular clouds. [PDF]
Zeng S +8 more
europepmc +1 more source

