The young spiral features of the Large Magellanic Cloud seen in the far-infrared

Details The young spiral features of the Large Magellanic Cloud seen in the far-infrared The young spiral features of the Large Magellanic Cloud seen in the far-infrared

Mar 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991mnras.249p...1l&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 249, March 1, 1991, p. 1P-3P.

Astronomy and Astrophysics

Astronomy

6

Far Infrared Radiation, Galactic Evolution, Magellanic Clouds, Spiral Galaxies, Black Body Radiation, Dark Matter, Infrared Astronomy Satellite, Ionized Gases, Star Formation

Scientific paper

Spiral features with ages of 10 Myr or less in the LMC are briefly characterized on the basis of an IRAS 100-micron contour map and grey-scale image. Previously known spiral features, centered around the H II complex 30 Dor, are revealed by extensive regions of blackbody-emitting dust, which also indicate the presence of additional features. The formation of the young spiral features is explained in terms of the stochastic star-formation model of Gerola and Seiden (1978) and Canto et al. (1980).

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