Results 121 to 130 of about 440 (199)
Discovering the sky at the longest wavelengths with a lunar orbit array. [PDF]
Chen X +6 more
europepmc +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
Dynamics of OH masers in regions of star formation I
A mathematical model for the explanation of OH masers in regions of star formation is presented. The model is based on the assumption that grains of different sizes are present at the border of the HII regions where they are exposed to the heat- and ...
H. Spiecker, T. Thissen, P. Andresen
core +1 more source
Sea surface brightness spectral anomalies from a Honolulu municipal outfall have been detected from space satellites in 200 km2 areas extending 20 km from the wastewater diffuser (Leung and Gibson 2004, Bondur 2005, Keeler et al.
Carl H. Gibson +3 more
doaj
SiO, <sup>29</sup>SiO, and <sup>30</sup>SiO emission from 67 oxygen-rich stars. A survey of 61 maser lines from 7 to 1 mm. [PDF]
Rizzo JR, Cernicharo J, Garoía-Miró C.
europepmc +1 more source
Maser radiation from astrophysical jets
Electromagnetic radiation from jets is normally considered to be incoherent synchrotron emission. Some aspects of radiation from both stellar and extragalactic jets could, however, be due to coherent emission mechanisms. Coherent radiation mechanisms have the advantage of being able to account for the high brightness temperatures inferred from some ...
Bingham, R +4 more
openaire +1 more source
Yebes 40 m radio telescope and the broad band NANOCOSMOS receivers at 7 mm and 3 mm for line surveys. [PDF]
Tercero F +25 more
europepmc +1 more source
Finding the Ionospheric Fluctuations Reflection in the Pulsar Signals' Characteristics Observed with LOFAR. [PDF]
Błaszkiewicz LP +6 more
europepmc +1 more source
Simultaneous VLBI Astrometry of H2O and SiO Masers toward the Semiregular Variable R Crateris
We obtained, for the first time, astrometrically registered maps of the 22.2 GHz H2O and 42.8, 43.1, and 86.2 GHz SiO maser emission toward the semiregular b-type variable (SRb) R Crateris, at three epochs (2015 May 21, and 2016 January 7 and 26) using ...
Yang, H. +19 more
core +1 more source

