Results 41 to 50 of about 2,871 (139)
Polarization properties of OH masers in AGB and post-AGB stars
Context: Ground-state OH maser emission from late-type stars is usually polarized and remains a powerful probe of the magnetic field structure in the outer regions of circumstellar envelopes if observed with high angular and spectral resolutions ...
Amiri +54 more
core +2 more sources
Milliarcsecond VLBI maps of regions containing 6.7 GHz methanol maser emission have lead to the recent discovery of ring-like distributions of maser spots and the plausible hypothesis that they may be tracing circumstellar disks around forming high mass ...
Anna Bartkiewicz +21 more
core +1 more source
Circumstellar water vapour in M-type AGB stars: Constraints from H2O(1_10 - 1_01) lines obtained with Odin [PDF]
Aims: Spectrally resolved circumstellar H2O(1_10 - 1_01) lines have been obtained towards three M-type AGB stars using the Odin satellite. This provides additional strong constrains on the properties of circumstellar H2O and the circumstellar envelope ...
Aa. Sandqvist +64 more
core +2 more sources
Phase–Referencing Observations of Galactic Circumstellar Masers [PDF]
AbstractTwo projects are discussed in which a phase referencing technique is used to determine stellar parallaxes and/or proper motions by means of the circumstellar masers. The observations are special in the sense that both continuum and line sources need to be detected.
Huib Jan van Langevelde +4 more
openaire +1 more source
Investigating Asymmetry Development from SiO to H2O Maser Regions in VX Sagittarii
Simultaneous very-long-baseline interferometry monitoring observations of H _2 O and SiO masers toward VX Sagittarii were conducted from 2014 February to 2019 January.
Dong-Hwan Yoon +4 more
doaj +1 more source
8 pages. 1 figure. Proceedings of the 7th European VLBI Network Symposium held in Toledo, Spain on October 12-15, 2004. Editors: R. Bachiller, F. Colomer, J.-F. Desmurs, P. de Vicente (Observatorio Astronomico Nacional), p. 169-176.
openaire +2 more sources
We investigated whether “velocity excess” in circumstellar maser lines can diagnose the earliest evolutionary phases of water fountains (WFs). Here, we define “velocity excess” as maser emission (e.g., H _2 O 22.235 GHz or OH 1665/1667 MHz) detected at ...
Jia-Yong Xie +2 more
doaj +1 more source
Mapping the circumstellar SiO maser emission in R Leonis [PDF]
accepted for publication in A& ...
Soria-Ruiz, R. +4 more
openaire +2 more sources
Equatorial Enhancement in the Dustiest OH/IR Stars in the Galactic Bulge
We have detected the 10 μ m silicate feature and the 11.3 μ m crystalline forsterite feature in absorption in 21 oxygen-rich asymptotic giant branch stars in the Galactic bulge.
Steven R. Goldman +4 more
doaj +1 more source
An astrophysical MASER (Microwave Amplification by Stimulated Emission of Radiation) is a source of stimulated spectral line emission. Maser emission is observed from the circumstellar envelopes of evolved stars, molecular clouds/star-forming regions ...
Humphreys, Elizabeth
core +1 more source

