Properties of star formation in the spiral arms of barred galaxies
Properties of star formation in the spiral arms of barred galaxies
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Publisher
Dordrecht: Springer Nature B.V
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Language
English
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Publisher
Dordrecht: Springer Nature B.V
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Contents
It is assumed that the two-fold disc-wide symmetry of spirals is caused by density waves, but also the potential of a bar component may have a significant influence on structural properties. The strength of the bar component appears to be anti-correlated with the degree of symmetry of star-forming regions in the spiral arms (Rozas et al., 1998). We...
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Full title
Properties of star formation in the spiral arms of barred galaxies
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TN_cdi_proquest_miscellaneous_27948013
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_27948013
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ISSN
0004-640X
E-ISSN
1572-946X
DOI
10.1023/A:1024088214799
