Hostname: page-component-78c5997874-8bhkd Total loading time: 0 Render date: 2024-11-02T19:25:36.677Z Has data issue: false hasContentIssue false
  • English
  • Français

New Evidence for Non-Cosmological Redshift

Published online by Cambridge University Press:  25 May 2016

Yaoquan Chu  and
Xingfen Zhu
Yaoquan Chu
Affiliation:
Center for Astrophysics, Univ. of Sci. and Tech. of China Hefei, Anhui 230026, China
Xingfen Zhu
Affiliation:
Center for Astrophysics, Univ. of Sci. and Tech. of China Hefei, Anhui 230026, China

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Recently Arp (1997) has published a list of x-ray emitting blue stellar objects (BSO) around 24 Seyfert galaxies. Herewith we present our optical identification of 5 BSOs in the field NGC3516 obtained on April 4-5, 1997 using the 2.16m telescope at Xinlong Station, Beijing Astronomical Observatory. One of the objects Q1107+7232 with z=2.10 (θ = 4.34′, θ is the angular distance from the center of NGC3516) is already listed in the Hewitt-Burbidge Catalog (1993). We find the other four objects are all quasars: Q1108+7226 with z=0.328 (θ = 11.23′); Q1106+7244, z=0.690 (θ = 10.23′); Q1105+7242, z=0.930, (θ = 10.990; QH05+7238, z=1.399 (θ = 7.42′) Q1107+7232, z=2.10 (θ = 4.34′)

Type
V. Cosmological Models
Information
Symposium - International Astronomical Union , Volume 183: Cosmological Parameters and the Evolution of the Universe , 1999 , pp. 296
Copyright
Copyright © Kluwer 1999 

References

Arp, H., (1997), AAp., 319, p.33.Google Scholar
Zhu, X. and Chu, Y., (1990), Acta Astronomica Sinica, 31, p.132.Google Scholar