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Observational Properties of SiO Masers in the Galactic Bulge IRAS Sources

Published online by Cambridge University Press:  25 May 2016

H. Izumiura
H. Izumiura*
Affiliation:
SRON Laboratory for Space Research Groningen, Landleven 12, P.O. Box 800, 9700 AV Groningen, The Netherlands

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We surveyed 313 color-selected IRAS sources in the Bulge in the SiO J=1−0 (v=1, 2) lines with the Nobeyama 45m telescope, which resulted in 222 detections (Nakada et al. 1992; Izumiura et al. 1994ab). The detection rates exceeded 80% for the brighter samples (Table 1). We discuss the observed SiO maser characteristics and the implications of the obtained 1-v diagram.

Type
Chapter 4: Is there a Consistent Picture of the Inner kpc of the Milky Way?
Information
Symposium - International Astronomical Union , Volume 169: Unsolved Problems of the Milky Way , 1996 , pp. 341 - 342
Copyright
Copyright © Kluwer 1996 

References

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