Dark nebulae in the Magellanic Clouds

Details Dark nebulae in the Magellanic Clouds Dark nebulae in the Magellanic Clouds

Oct 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974apj...193...63v&link_type=abstract

Astrophysical Journal, vol. 193, Oct. 1, 1974, pt. 1, p. 63, 64. Research supported by the National Research Council of Canada.

Physics

24

Cosmic Dust, Electromagnetic Absorption, Interstellar Gas, Magellanic Clouds, Nebulae, Astronomical Photography, Cloud Physics, Heavy Elements, Hydrogen Clouds, Interstellar Extinction

Scientific paper

Curtis Schmidt plates of the Magellanic Clouds show that both the LMC
and the SMC contain dark nebulae. The dark clouds in the Large Cloud
are, however, much more prominent than are those in the Small Cloud. It
is suggested that this difference is due to the fact that the SMC gas
has a lower heavy-element content than does the gas in the LMC.

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