The nature of dust grains in the clouds of Magellan - 8-13 micron spectra of LMC N44A and SMC N88A

Details The nature of dust grains in the clouds of Magellan - 8-13 micron spectra of LMC N44A and SMC N88A The nature of dust grains in the clouds of Magellan - 8-13 micron spectra of LMC N44A and SMC N88A

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987mnras.228..269r&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 228, Sept. 1, 1987, p. 269-275. SERC-supported research

Astronomy and Astrophysics

Astronomy

7

Astronomical Photometry, Cosmic Dust, Grain Size, Infrared Spectra, Magellanic Clouds, Silicates, Hydrogen Clouds, Milky Way Galaxy

Scientific paper

The authors present 8 - 13 μm spectrophotometry of two Magellanic cloud H II regions, LMC N44A and SMC N88A. The former shows a prominent silicate emission feature and resembles many galactic H II regions, whilst the latter shows no evidence of silicate dust. The implications for the composition of dust particles in the clouds and the species responsible for the 2200 Å feature are discussed.

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