Dust and Gas in the Small Magellanic Cloud

Dust and Gas in the Small Magellanic Cloud

Here we present four IRAS high resolution images of the Small Magellanic Cloud, as reconstructed by the HIRAS program using the Pyramid Maximum Entropy method (Bontekoe et al. 1994). (HIRAS is not to be confused with HiRes (Aumann et al. 1990).) The images show much more detail than in Schwering &am...

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Veröffentlicht in:Symposium - International Astronomical Union 1999, Vol.190, p.122-123
Hauptverfasser: Bontekoe, Tj.R., Kester, D.J.M., Stanimirović, S., Staveley–Smith, L., van der Hulst, J.M.
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Sprache:eng
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Zusammenfassung:Here we present four IRAS high resolution images of the Small Magellanic Cloud, as reconstructed by the HIRAS program using the Pyramid Maximum Entropy method (Bontekoe et al. 1994). (HIRAS is not to be confused with HiRes (Aumann et al. 1990).) The images show much more detail than in Schwering & Israel (1990). Dust temperatures range from 25–41 K (Stanimirović et al. in prep).
ISSN:0074-1809
DOI:10.1017/S0074180900117589