Abstract
The use of TAURUS-2 (a Fabry-Perot imaging spectrograph) for the study of the kinematics and the dynamics of giant extragalactic H II regions in nearby galaxies is discussed. The technical aspects of the instrument, together with the procedures adopted for data analysis and reduction, and some of the first scientific results of our program are also presented.
Original language | English |
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Pages (from-to) | 267-270 |
Number of pages | 4 |
Journal | Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias |
Volume | 3 |
State | Published - 1995 |
Externally published | Yes |
Event | 5th Mexico-Texas Conference on Astrophysics: Gaseous Nebulae and Star Formation - Tequesquitengo, Mor, Mexico Duration: 3 Apr 1995 → 5 Apr 1995 |
Keywords
- HII regions
- ISM: kinematics and dynamics