A Search for 43.122 GHz SiO Emission from Symbiotic Stars-Reference-Cited by-同舟云学术

A Search for 43.122 GHz SiO Emission from Symbiotic Stars

Published:1987 Issue:1 Volume:7 Page:50-54
ISSN:1323-3580
Container-title:Publications of the Astronomical Society of Australia
language:en
Short-container-title:Publ. Astron. Soc. Aust.

Author:

Hall P. J.,Wark Robin M.,Wright Alan E.

Abstract

AbstractDuring the second half of 1986 tests were made of a new Q-band (43 GHz) receiver designed for the Parkes radio telescope. As part of the trial observation program 12 symbiotic stars were examined for SiO maser emission. No significant new emission was detected from any of the candidates, although several previously known SiO sources (including one symbiotic star) were confirmed. We conclude that potential SiO maser action near the Mira star in most symbiotic systems is prevented by the presence of the hot companion star.

Publisher

Cambridge University Press (CUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference9 articles.

1. Observations of SiO maser sources at 43.122 GHz

2. Maser Emission as a Tool to Study Mass Loss from Evolved Stars

3. Millimetre Wavelength performance of the new 16.7m surface of the Parkes Radio Telescope

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