Abstract
The GHz-Peaked-Spectrum (GPS) radio sources are powerful (L radio ≈ 1045 erg sec−1) and compact (10–100 mas, 10–1000 parsecs) sources characterized by a simple convex spectrum which peaks near 1 GHz (O’Dea et al. 1991 and references therein).
This is a preview of subscription content, log in via an institution to check access.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
References
Dallacasa D., et al. 1995 Astron. Astrophys., 205, 27
Fanti, C., Fanti, R., Dallacasa, D., Schilizzi, R. T., Spencer, R. E., and Stanghellini, C., 1995, Astron. As trophy s., 302, 317
O’Dea, C.P., Baum, S.A., Stanghellini, C., 1991, Astrophys. 380, 66
Readhead A. C. S., et al. 1994, CERS meeting
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1996 International Astronomical Union
About this paper
Cite this paper
Stanghellini, C., O’Dea, C.P., Baum, S.A., Dallacasa, D., Fanti, R., Fanti, C. (1996). A VLBI Study of GHZ-Peaked-Spectrum Radio Sources. In: Ekers, R., Fanti, C., Padrielli, L. (eds) Extragalactic Radio Sources. International Astronomical Union, vol 175. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-0295-4_25
Download citation
DOI: https://doi.org/10.1007/978-94-009-0295-4_25
Publisher Name: Springer, Dordrecht
Print ISBN: 978-0-7923-4122-2
Online ISBN: 978-94-009-0295-4
eBook Packages: Springer Book Archive