Dickel, J.R., Angerhofer, P.E., Strom, R.G., Smith, M.D. (1981) CTB80: a galactic radio source with directed jets. Vistas in Astronomy, 25 (PART 1). pp. 127-135. ISSN 0083-6656. (doi:10.1016/0083-6656(81)90053-2) (The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided) (KAR id:50166)
| The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided. | |
| Official URL: http://dx.doi.org/10.1016/0083-6656(81)90053-2 |
|
| Additional URLs: |
|
Abstract
The galactic radio source CTB80 shows several remarkable jets which can be traced outward to over 30pc from a point less than 0.1 pc within a central core. If the object is associated with a supernova of 1408 then the jets must move out at a velocity of 0.2 c but the morphology of the whole source suggests a significant proper motion of the central object which argues for an older age. In this case continuous ejection into the jets must have occurred for tens of thousands of years. A model involving a supernova explosion ejecting several massive path-cutting fragments is quantitatively explored, and found to be plausible.
| Item Type: | Article |
|---|---|
| DOI/Identification number: | 10.1016/0083-6656(81)90053-2 |
| Subjects: | Q Science > QB Astronomy > QB460 Astrophysics |
| Institutional Unit: | Schools > School of Engineering, Mathematics and Physics > Physics and Astronomy |
| Former Institutional Unit: |
Divisions > Division of Natural Sciences > Physics and Astronomy
|
| Depositing User: | Giles Tarver |
| Date Deposited: | 11 Aug 2015 10:44 UTC |
| Last Modified: | 20 May 2025 09:39 UTC |
| Resource URI: | https://kar.kent.ac.uk/id/eprint/50166 (The current URI for this page, for reference purposes) |
- Export to:
- RefWorks
- EPrints3 XML
- BibTeX
- CSV
- Depositors only (login required):

https://orcid.org/0000-0002-4289-5952
Altmetric
Altmetric