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Simultaneity and Flux Bias between 43 and 86 GHz SiO Masers

Published online by Cambridge University Press:  16 July 2018

Michael C. Stroh ,
Ylva M. Pihlström  and
Lorant O. Sjouwerman
Michael C. Stroh
Affiliation:
Department of Physics & Astronomy, The University of New Mexico, Albuquerque, NM 87131 email: mstroh@unm.edu
Ylva M. Pihlström
Affiliation:
Department of Physics & Astronomy, The University of New Mexico, Albuquerque, NM 87131 email: mstroh@unm.edu National Radio Astronomy Observatory
Lorant O. Sjouwerman
Affiliation:
National Radio Astronomy Observatory
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Abstract

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Using quasi-simultaneous observations of 86 stars with known SiO maser emission, we searched for systematic differences between the strengths of the 43 and 86 GHz v=1 maser lines. Although for individual stars there is wide scatter between the line strengths spanning nearly an order of magnitude, there is no evidence of a systematic difference between these line strengths for the entire sample.

Keywords

Masersstars: late-typeinfrared: starsradio lines: stars
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 13 , Symposium S336: Astrophysical Masers: Unlocking the Mysteries of the Universe , September 2017 , pp. 399 - 400
Copyright
Copyright © International Astronomical Union 2018 

References

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