Solar wind and stellar jets, from newtonian to relativistic ones

• Type: Article in International Conference Proceedings Book
• Date: 2007

Authors

Sauty, C (Author) Other; Lima, JJG (Author) FCUP; Tsinganos, K (Author) Other; Aibeo, A (Author) Other; Meliani, Z (Author) Other; Vlahakis, N (Author) Other

Conference proceedings International

Title: Fifty Years of Romanian Astrophysics

International Conference on Fifty Years of Romanian Astrophysics

Bucharest, ROMANIA, SEP 27-30, 2006

Indexing

ISI Web of Knowledge - 0 Citations

Scopus - 0 Citations

Scientific classification

FOS: Natural sciences > Physical sciences

Other information

Authenticus ID: P-005-71Y

Abstract (EN): In parallel to the development of numerical simulations, analytical solutions for modelling the acceleration and the collimation of winds and jets have been proposed. We present here how meridionally self-similar solutions can be used to model the solar wind using Ulysses data at solar minimum. Such solutions may also be adapted to explain the formation core or spine jets in classical and weak TTauri stars (class II and III young stellar jets) as well as relativistic jet cores from AGN. The criterion for collimation explains how the jet evolves towards awind as the star approaches the main sequence. A similar scenario could explain the winds from Seyfert galaxies by opposition to the powerful jets from Fanaroff Riley sources.

Language: English

Type (Professor's evaluation): Scientific