On the Nature of Variability of Extragalactic Radio Sources: Fundamental Ideas by I.S. Shklovsky |
| |
| Authors: | Yu A Kovalev Y Y Kovalev |
| |
| Institution: | (1) Astro Space Center of the Lebedev Physical Institute Profsoyuznaya 84/32, 117810 Moscow, Russia;(2) Moscow State University Vorobjevy gory, 119899 Moscow, Russia |
| |
| Abstract: | The majority (maybe all) of proposed relativistic and non-relativistic models for variable extragalactic radio sources are based on the same general ideas proposed in the early model by Shklovsky (1960, 1965) – in particular, that the variability is caused by the synchrotron emission of magnetized clouds during their expansion. This model was a "standard" or "canonical" model for more than 20 years. One of the models that uses its ideas and approach is the "hedgehog" model, in which clouds or jets emit and expand in the strong external radial magnetic field of the nucleus of the source. This model has been suggested for a long time, but recent new results comparing it's predictions with observations of multifrequency spectra – especially, instantaneous spectra of many variable sources – and with the typical VLBI structure of compact objects have given strong new arguments in it's favour. The nature of the variability can be satisfactory explained by the hedgehog jet model for many variable and compact extragalactic radio sources. Thus, following up the ideas of I.S. Shklovsky, we conclude that the observed spectra and structure of compact sources can be caused by the synchrotron emission of a quasi-stationary jet in a longitudinal magnetic field, and the nature of variability can be explained by the variable ejection of the continious jet from the nucleus. |
| |
| Keywords: | |
| 本文献已被 SpringerLink 等数据库收录！ |
|
