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Molecular Gas, Dust and Star Formation in the Barred Spiral NGC 5383

ASTROPHYSICAL JOURNAL, no. 1 (2000): 221-237

Cited by: 94|Views9

Abstract

We have mapped the barred spiral NGC 5383 using the Berkeley-Illinois-Maryland Association millimeter-wave array for observations of CO (J = 1-0), the Palomar 1.5 m telescope for H alpha and optical broadband, and the Kitt Peak 1.3 m telescope for near-IR broadband. We compare the observed central gas and dust morphology to the prediction...More

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