Emission-line stars in the Large Magellanic Cloud - Spectroscopy and infrared photometry

Details Emission-line stars in the Large Magellanic Cloud - Spectroscopy and infrared photometry Emission-line stars in the Large Magellanic Cloud - Spectroscopy and infrared photometry

Dec 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...210..666a&link_type=abstract

Astrophysical Journal, vol. 210, Dec. 15, 1976, pt. 1, p. 666-669.

Astronomy and Astrophysics

Astronomy

36

Astronomical Spectroscopy, Binary Stars, Emission Spectra, Infrared Astronomy, Infrared Photometry, Magellanic Clouds, Stellar Spectrophotometry, Astronomical Photometry, Forbidden Bands, Infrared Scanners, Iron, Late Stars, Line Spectra, Stellar Envelopes, Stellar Spectra

Scientific paper

Twelve emission-line stars in the Large Magellanic Cloud have been
observed using an infrared (JHKL) photometer and an image-dissector
scanner operating in the visible region. Several of these have
pronounced infrared excesses. The correlation of forbidden Fe II
emission and infrared excess appears valid in the LMC.

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