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A Possible Molecular Counterpart to the G359.54+0.18 Non-Thermal Filaments

Published online by Cambridge University Press:  23 September 2016

John Bally ,
Farhad Yusef-Zadeh  and
J. M. Hollis
John Bally
Affiliation:
AT&T Bell Laboratories, Holmdel, New Jersey
Farhad Yusef-Zadeh
Affiliation:
AT&T Bell Laboratories, Holmdel, New Jersey Space Data and Computing Division, NASA/Goddard Space Flight Center
J. M. Hollis
Affiliation:
Space Data and Computing Division, NASA/Goddard Space Flight Center

Abstract

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We present new 30″ resolution J=2–1 12CO observations of the molecular gas located close to a group of non-thermal radio emitting filaments recently detected near the Galactic center (Bally and Yusef-Zadeh, 1989). The new data provide some support for the association of the non-thermal filaments G359.54+0.18 with the projected edge of a molecular cloud.

Type
Observations of Discrete Sources
Information
Symposium - International Astronomical Union , Volume 136: The Galactic Center , 1989 , pp. 189 - 193
Copyright
Copyright © Kluwer 1989 

References

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