Are CSO host-galaxies undergoing merging?
| dc.creator | Liu, Xiang | |
| dc.date | 2000-10-14 | |
| dc.date.accessioned | 2026-07-07T01:55:59Z | |
| dc.date.available | 2026-07-07T01:55:59Z | |
| dc.description | The galaxy-type CSO (compact symmetric objects) rate from an intermediate large sample PR+CJ1 is found to be consistent with the Sb-Sb merger rate of 4.6% in redshift z<1. The CSO detection rate seems going down when the sample size is increasing, which could not reach the high merger rate in z>1, yet no deep VLBI sample in z>1 is available now. | |
| dc.description | 4 pages, 2 figures, to be appeared in the "Proceedings of the 5th EVN Symposium", Eds. J. Conway, A. Polatidis, R. Booth, Onsala Space Observatory, Chalmers Technical University, Gothenburg, Sweden (2000) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0010281 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0010281 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/1846 | |
| dc.subject | Astrophysics | |
| dc.title | Are CSO host-galaxies undergoing merging? | |
| dc.type | text |