Spirals – classified by size of central bulge
•tightness of spiral pattern correlated with bulge size
•arms more knotty Sa ® Sc
•i/s gas (21 cm (H) & molecular line radiation) increases Sa ® Sc
•A & G stars in disk ® whitish color
•new O & B stars b(+ nebulae) in arms ® bluish color
•Barred spirals – SBa ® SBc (massive dark matter halo ® no bar?)
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