Emission-line objects in the Large Magellanic Cloud. Observations obtained with the FLAIR system.
Abstract
The FLAIR multi-object, fibre-coupled, spectroscopy system on the UK Schmidt Telescope has been used to observe a miscellany of emission-line objects in the Large Magellanic Cloud. The observations have been used to demonstrate the system's ability to provide quantitative measurements of emission-line objects. A comparison is made with published data where possible, and new classifications and measurements are presented.
- Publication:
-
Astronomy and Astrophysics Supplement Series
- Pub Date:
- June 1992
- Bibcode:
- 1992A&AS...93..495M
- Keywords:
-
- Astronomical Spectroscopy;
- Emission Spectra;
- Magellanic Clouds;
- Schmidt Telescopes;
- Stellar Spectrophotometry;
- B Stars;
- Data Reduction;
- H Ii Regions;
- Planetary Nebulae;
- Red Shift;
- Wolf-Rayet Stars;
- Astronomy