Results 81 to 90 of about 2,871 (139)

Single-dish monitoring of circumstellar water masers

open access: yes, 2002
6 pages. Contribution to a workshop held in Cagliari (I), Nov. 2001: "SRT: The Impact of Large Antennas on Radioastronomy and Space Science". Proceedings to be published as a special issue of the Publ.
Brand J., Baldacci L., Engels D.
openaire   +3 more sources

Interferometric confirmation of "water fountain" candidates

open access: yes, 2017
Water fountain stars (WFs) are evolved objects with water masers tracing high-velocity jets (up to several hundreds of km s$^{-1}$). They could represent one of the first manifestations of collimated mass-loss in evolved objects and thus, be a key to ...
Bendjoya, Philippe   +6 more
core   +1 more source

The three-dimensional structure of a circumstellar maser

open access: yesThe Astrophysical Journal, 1984
A 900-day observation of the line profile of the unusual 1667 MHz OH maser in the bipolar nebula OH 231.8+4.2 has indicated that it varies sinusoidally by a factor of about 3, with a period of 684 + or - 40 days. This is in agreement with recent IR observations. The phase of the variations varies strongly with velocity.
P. F. Bowers, M. Morris
openaire   +1 more source

Interstellar nitrile anions: Detection of C<sub>3</sub>N<sup>-</sup> and C<sub>5</sub>N<sup>-</sup> in TMC-1. [PDF]

open access: yesAstron Astrophys, 2020
Cernicharo J   +7 more
europepmc   +1 more source

Astrometry of Water Maser Sources in Nearby Molecular Clouds with VERA - II. SVS 13 in NGC 1333

open access: yes, 2007
We report on the results of multi-epoch VLBI observations with VERA (VLBI Exploration of Radio Astrometry) of the 22 GHz H2O masers associated with the young stellar object SVS 13 in the NGC 1333 region.
Bushimata, Takeshi   +27 more
core   +1 more source

Detection of vibrationally excited HC<sub>7</sub>N and HC<sub>9</sub>N in IRC+10216 <sup>⋆</sup>. [PDF]

open access: yesAstron Astrophys, 2020
Pardo JR   +10 more
europepmc   +1 more source

The Maser Emitting Structure and Time Variability of the SIS Lines <i>J</i> = 14 - 13 and 15 - 14 in IRC+10216. [PDF]

open access: yesAstrophys J, 2018
Fonfría JP   +10 more
europepmc   +2 more sources

First VLBI mapping of circumstellar 29SiO maser emission

open access: yes, 2005
4 pages, 2 figures.
Soria-Ruiz, R.   +5 more
openaire   +2 more sources

Formation and Evolution of Disks Around Young Stellar Objects. [PDF]

open access: yesSpace Sci Rev, 2020
Zhao B   +11 more
europepmc   +1 more source

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