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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: [email protected]
W. Tian
Affiliation:
National Astronomical Observatories, CAS, Beijing, China, Email: [email protected]
H. Su
Affiliation:
National Astronomical Observatories, CAS, Beijing, China, Email: [email protected]
D. Wu
Affiliation:
National Astronomical Observatories, CAS, Beijing, China, Email: [email protected]
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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

Anderson, L. D., Bania, T. M., Balser, D. S., & Rood, R. T. 2012, ApJ, 754, 62Google Scholar
Anderson, L. D., Bania, T. M., Jackson, J. M., Clemens, D. P., Heyer, M., Simon, R., Shah, R. Y., & Rathborne, J. M. 2009, ApJS, 181, 255Google Scholar
Paron, S. & Giacani, E. 2010, A&A, 509, L4Google Scholar
Tian, W. W. & Leahy, D. A. 2013, ApJ, 769L, 17CrossRefGoogle Scholar
Williams, J. P. & Maddelena, R. J. 1996, ApJ, 464, 247Google Scholar