other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
2011MNRAS.411..849G - Mon. Not. R. Astron. Soc., 411, 849-858 (2011/February-3)
On the source of dense outflows from T Tauri stars – III. Winds driven from the star–disc shear layer.
GOMEZ DE CASTRO A.I. and VON REKOWSKI B.
Abstract (from CDS):
In addition, it is shown that the non-stationary nature of star-disc winds produce a flickering of the profile during quiescence with variations in the line flux of about 10 per cent. At outburst, accretion signatures appear in the profiles together with an enhancement of the wind, producing the correlation between accretion and outflow as reported from RU Lup, AA Tau and RW Aur observations.
Abstract Copyright: 2010 The Authors. Journal compilation2010 RAS
Journal keyword(s): stars: formation - stars: variables: T Tauri, Herbig Ae/Be - stars: winds, outflows - ISM: jets and outflows
Simbad objects: 8
To bookmark this query, right click on this link: simbad:2011MNRAS.411..849G and select 'bookmark this link' or equivalent in the popup menu