Young Powerful Radio Sources and their Evolution

Fanti, R.

doi:10.1007/1-4020-2406-1_9

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Polarization2

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2016

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Cited by 1 publication

(2 citation statements)

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“…Cotton et al (2003) found that small radio sources are unpolarized in the NVSS at 1.4 GHz ( Fig. 2.7), while at higher frequencies sources with size of about a few kpc start to show some fractional polarization at progressively smaller projected linear sizes (Fanti et al, 2004).…”

Section: Polarizationmentioning

confidence: 96%

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Multifrequency VLBA observations of two compact symmetric objects

2016

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We present the results of multifrequency VLBA observations of J1944+5448 and J0111+3906. These sources are compact symmetric objects, completely embedded in the narrow line region of the host galaxy. Multi-epoch observations allowed us to derive the hot-spot separation speed that was used to estimate the kinematic age of both sources. Their asymmetric shape is likely due to an inhomogeneous ambient medium with which these sources interact. Finally we present the results on the spectral analysis of J0111+3906 whose spectrum is ﬁtted with either a synchrotron self-absorption mechanism or a free free absorption model

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Section: Polarizationmentioning

confidence: 96%

“…This implies that these compact radio sources are generally surrounded by a very dense ionized medium (Fanti, 2004).…”

Section: Polarizationmentioning

confidence: 99%