Investigation of the galactic rotation from the 21 cm line
The maximum likelyhood method is used for study of galactic rotation which utilises the whole 21 cm line profile. The rotation curve is obtained in the region from R = 0.4 R, up to 2.3 R, and we do not find evidence for a fall-off bellow a flat rotation curve.
- Petrovskaya, I. V.
- space research
- galactic rotation
- 21 cm line profile
- model:article
- Petrovskaya, I. V.
- space research
- galactic rotation
- 21 cm line profile
- model:article
- http://creativecommons.org/publicdomain/mark/1.0/
- false
- policy:public
- 307-309
- Publications of the Astronomical Institute of the Academy of Sciences of the Czech Republic | 1987 Volume:63-70 | Number:69
- uuid:0557d549-9d2e-4213-a7f9-1fe54f00ba51
- https://cdk.lib.cas.cz/client/handle/uuid:0557d549-9d2e-4213-a7f9-1fe54f00ba51
- uuid:0557d549-9d2e-4213-a7f9-1fe54f00ba51
- bez média
- svazek
- ces
- cze
- Czech Republic
- 2021-06-01T12:19:28.026Z
- 2021-06-01T12:19:28.026Z