Emission-line objects in the Large Magellanic Cloud - Observations obtained with the FLAIR system

Details Emission-line objects in the Large Magellanic Cloud - Observations obtained with the FLAIR system Emission-line objects in the Large Magellanic Cloud - Observations obtained with the FLAIR system

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26as...93..495m&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 93, no. 3, June 1992, p. 495-507. Research supported by SERC

Astronomy and Astrophysics

Astrophysics

10

Astronomical Spectroscopy, Emission Spectra, Magellanic Clouds, Schmidt Telescopes, Stellar Spectrophotometry, B Stars, Data Reduction, H Ii Regions, Planetary Nebulae, Red Shift, Wolf-Rayet Stars

Scientific paper

The FLAIR multi-object, fiber-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.

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