Abstract
We discuss recent work on massive star-formation efficiency parameters on 1 kpc scales in grand-design spiral galaxies. The fact that in two galaxies studies in detail, M51 and NGC 4321, the massive star-formation efficiency in the arms is larger than that outside the arms can be seen as evidence for large-scale triggering of the star formation in the arms, probably induced by a density wave system. We discuss several possible systematic effects, but infer that the conclusions on triggering are sound.
Original language | English |
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Title of host publication | In: Physics of the Gaseous and Stellar Disks of the Galaxy - ASP Conf Series 66 |
Publisher | Astronomical Society of the Pacific |
Pages | 329-336 |
ISBN (Print) | 0-937707-85-6 |
Publication status | Published - 1994 |