Summary: A&A manuscript no.
(will be inserted by hand later)
Your thesaurus codes are:
02.12.1; 02.12.3; 02.20.1; 08.01.2; 08.03.3; 08.12.1 Gl 616.2
ASTRONOMY
AND
ASTROPHYSICS
April 17, 2000
The Contribution of the Micro­Turbulent Velocity on the
Modelling of Chromospheric Lines in Late Type Dwarfs ?
D. Jevremovi'c 1;2 , J.G. Doyle 1 , and C.I. Short 3
1 Armagh Observatory, College Hill, Armagh BT61 9DG, N. Ireland
email: djc@star.arm.ac.uk jgd@star.arm.ac.uk
2 Belgrade Observatory, Volgina 7, 11160 Belgrade 74, Yugoslavia
3 Department of Physics & Astronomy, University of Georgia, Athens, GA, 30602­2451, USA
receive date, accepted date
Abstract. We discuss the influence of the non­thermal
velocity (micro­turbulence) on the formation of chromo­
spheric lines in the atmospheres of late type dwarfs. A
review of previous work shows a variety of different ap­

Source: Armagh Observatory

Collections: Physics