SiO Masers in Mira with ALMA Long Baselines
The effect of binary companions on the near-circumstellar environment of AGB stars is an open-question. Using ALMA long baseline data, we have investigated this region of Mira A using SiO emission.
Humphreys, Elizabeth +1 more
core +1 more source
I-VLBI of molecular masers [PDF]
Intense maser emissions of several molecular species (OH, CH3OH, H2O, SiO) are widely observed toward both star-formation regions and late-type stars.
PORCEDDU, Ignazio Enrico Pietro +1 more
core
The Maser Emitting Structure and Time Variability of the SIS Lines <i>J</i> = 14 - 13 and 15 - 14 in IRC+10216. [PDF]
Fonfría JP +10 more
europepmc +2 more sources
Circumstellar masers around oxygen-rich stars
The far-IR colors of bright oxygen-rich stars define a clear sequence from sources along the blackbody curve with temperatures above 2000 K, across a small gap at color temperatures in the range 1000-2000 K, down to temperatures of about 300 K, where stars are heavily obscured.
openaire +1 more source
OBSERVATIONS OF MASSIVE STAR-FORMING REGIONS WITH WATER MASERS: MID-INFRARED IMAGING
We present here a mid-infrared imaging survey of 26 sites of water maser emission. Observations were obtained at the Infrared Telescope Facility 3 m telescope with the University of Florida mid-infrared imager/spectrometer OSCIR, and the JPL mid-infrared
C. M. Telesco +3 more
core
High resolution magnetic field measurements in high-mass star-forming regions using masers
The bright and narrow spectral line emission of masers is ideal for measuring the Zeeman-splitting as well as for determining the orientation of magnetic fields in 3-dimensions around massive protostars.
Hutarawarakorn Kramer, B., +8 more
core +1 more source
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
Formation and Evolution of Disks Around Young Stellar Objects. [PDF]
Zhao B +11 more
europepmc +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
Astrometrically registered maps of H2O and SiO masers toward VX Sagittarii. [PDF]
Yoon DH +10 more
europepmc +1 more source

