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

1989 ◽  
Vol 120 ◽  
pp. 194-194
Author(s):  
A. Laval ◽  
M. Rosado ◽  
J. Boulesteix ◽  
Y.P. Georgelin ◽  
M. Marcelin ◽  
...  

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”).

2004 ◽  
Vol 21 (1) ◽  
pp. 79-80 ◽  
Author(s):  
Guo Wei-Hua ◽  
Huang Yong-Zhen ◽  
Lu Qiao-Yin ◽  
Yu Li-Juan

1995 ◽  
Vol 164 ◽  
pp. 438-438
Author(s):  
O.K. Sil'chenko

The central part of NGC 1052 has been observed at the prime focus of the 6m telescope with the Multi-Pupil Spectrophotometer equipped with a two-dimensional IPCS. Ninety-nine spectra over the central 14.5″x11″ are registered in the spectral range of λλ4700 – 5400 AA and are used to map ionized-gas velocities (by [OIII]λ5007) and to derive radial profiles of absorption-line equivalent width for MgIλA5175, FeIλ5270, and Hβ.


1990 ◽  
Vol 137 ◽  
pp. 267-270
Author(s):  
T.Yu. Magakyan ◽  
T.A. Movsessian

The results of spectral investigations of collimatee outflows from young stellar objects, including HL/XZ Tau, L723, Bernes 48, RNO 43N, CoKu Tau/1, obtained on 6-m telescope BTA with two-dimensional photon counting system in 1986-1988 are presented.


1999 ◽  
Vol 93 (2) ◽  
pp. 163-168 ◽  
Author(s):  
Masaki Kobayashi ◽  
Motohiro Takeda ◽  
Ken-Ichi Ito ◽  
Hiroshi Kato ◽  
Humio Inaba

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