Article contents
Interaction Between A Stellar Wind and the Ionized Gas in N120 (LMC)
Published online by Cambridge University Press: 12 April 2016
Extract
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
- Copyright
- Copyright © Springer-Verlag 1989
- 1
- Cited by