The interstellar lambda 4428 feature in the Large Magellanic Cloud

Details The interstellar lambda 4428 feature in the Large Magellanic Cloud The interstellar lambda 4428 feature in the Large Magellanic Cloud

Jan 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979a%26a....71..359b&link_type=abstract

Astronomy and Astrophysics, vol. 71, no. 3, Jan. 1979, p. 359-361.

Astronomy and Astrophysics

Astrophysics

7

Astronomical Spectroscopy, Interstellar Matter, Magellanic Clouds, Stellar Spectra, Supergiant Stars, Absorption Spectra, B Stars, Cosmic Dust, Line Spectra, Spectral Bands

Scientific paper

A search has been made for this interstellar absorption band in four B-type supergiant members of the LMC. Upper limits are derived which agree with predictions from the well-established galactic 4428-A/E(B-V) correlation. A previous report of anomalously strong 4428 A in this direction is shown to be in error, the overestimation probably being caused by stellar line interference.

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