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Kinematic Distance of Galactic Radio Objects

Published online by Cambridge University Press:  21 February 2014

H. Zhu ,
W. Tian ,
H. Su  and
D. Wu
H. Zhu
Affiliation:
National Astronomical Observatories, CAS, Beijing, China, Email: zhuhui@bao.ac.cn
W. Tian
Affiliation:
National Astronomical Observatories, CAS, Beijing, China, Email: zhuhui@bao.ac.cn
H. Su
Affiliation:
National Astronomical Observatories, CAS, Beijing, China, Email: zhuhui@bao.ac.cn
D. Wu
Affiliation:
National Astronomical Observatories, CAS, Beijing, China, Email: zhuhui@bao.ac.cn
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Abstract

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We briefly summarize the method of kinematic distances of Galactic radio objects and discuss the ambiguity in this method. Both Hi absorption and Hi self-absorption are effective tools to solve the kinematic distance ambiguity. We build the 21 cm Hi absorption spectrum of the complex G35.6-0.5, and suggest SNR G35.6-0.4, one component of the complex, is located at the near side distance of about 3.6 kpc.

Keywords

ISM: kinematics and dynamicsISM: supernova remnants
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S297: The Diffuse Interstellar Bands , May 2013 , pp. 232 - 234
Copyright
Copyright © International Astronomical Union 2014 

References

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