Hostname: page-component-7479d7b7d-q6k6v Total loading time: 0 Render date: 2024-07-13T19:06:47.726Z Has data issue: false hasContentIssue false
  • English
  • Français

Interaction Between A Stellar Wind and the Ionized Gas in N120 (LMC)

Published online by Cambridge University Press:  12 April 2016

A. Laval ,
M. Rosado ,
J. Boulesteix ,
Y.P. Georgelin ,
M. Marcelin ,
A. Greve ,
J. Larsen  and
A. Viale
A. Laval
Affiliation:
Observatoire de Marseille, France
M. Rosado
Affiliation:
Universidad Nacional Autónoma de México, México
J. Boulesteix
Affiliation:
Observatoire de Marseille, France
Y.P. Georgelin
Affiliation:
Observatoire de Marseille, France
M. Marcelin
Affiliation:
Observatoire de Marseille, France
A. Greve
Affiliation:
IRAM, Granada, Spain
J. Larsen
Affiliation:
Sterrewacht Leiden, Holand
A. Viale
Affiliation:
Observatoire de Marseille, France

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The western part of the nebula N120, in the LMC, was observed in Hα with the equipment CIGALE at ESO. This equipment consists mainly of a scanning Perot-Fabry interferometer and a two-dimensional photon counting system. The spectral step used here is 0.41 Ǡover free spectral range of 8.24 Ǡ. The total field of view of 7’ x 7’ is covered by 256 x 256 pixels (each pixel being there 2.6” x 2.6”).

Type
II. Mechanical Energy Sources
Information
International Astronomical Union Colloquium , Volume 120: Structure and Dynamics of the Interstellar Medium , 1989 , pp. 194
Copyright
Copyright © Springer-Verlag 1989