Hostname: page-component-586b7cd67f-dlnhk Total loading time: 0 Render date: 2024-11-30T02:30:57.615Z Has data issue: false hasContentIssue false
  • English
  • Français

Magnetic Field Strengths of GPS Radio Sources

Published online by Cambridge University Press:  25 May 2016

V. G. Panajyan
V. G. Panajyan*
Affiliation:
Byurakan Astrophysical Observatory, Armenia

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.

GHz peaked spectrum radio sources (GPS) are believed to be a subclass of compact steep spectrum radio sources (CSS) with high frequency spectral indices α < −0.5 (5 ˜ vα), linear sizes of pc to kpc scale and turnover spectra near 1GHz. Due to the work of many radioastronomers during the past two decades many properties of CSS and GPS radio sources at present are known (O'Dea,C.P. et al.1998, and references therein).

Type
III. AGN Theory and Models
Information
Symposium - International Astronomical Union , Volume 194: Activity in Galaxies and Related Phenomena , 1999 , pp. 324 - 326
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

Arthyukh, V. S., Hovhannissian, M. A., & Tyul'bashev, S. A. 1994, Pisma v AZh. 20, 178 Google Scholar
Arthyukh, V.S., Hovhannissian, M. A., & Tyul'bashev, S. A. 1994, Pisma v AZh. 20, 258 Google Scholar
Athreya, R. M., Kapahi, V. K., McCarthy, P.J., & van Breugel, W. 1997, MNRAS, 289, 525 Google Scholar
O'Dea, C. P., 1998, PASP, 110, 493 Google Scholar
O'Dea, C. P., & Baum, C. A. 1997, AJ, 113, 148 Google Scholar
Oort, M. J. A. 1988, A&A, 192, 42 Google Scholar
Panajyan, V. G. 1998, Astrofizika, 41, 377 Google Scholar
Slish, V. 1963, Nature, 199, 682 Google Scholar
Stanghellini, C., O'Dea, C. P., Dallacasa, D., Baum, S. A., Fanti, R., & Fanti, C. 1998, A&AS, 131, 303 Google Scholar
Williams, I. P. 1963, Nature, 200, 56 Google Scholar