Kinematic Distance of Galactic Radio Objects
Abstract
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.
- Publication:
-
The Diffuse Interstellar Bands
- Pub Date:
- February 2014
- DOI:
- 10.1017/S1743921313015937
- Bibcode:
- 2014IAUS..297..232Z
- Keywords:
-
- ISM: kinematics and dynamics;
- ISM: supernova remnants