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- W1799843663 abstract "The NRO-OVRO CO imaging survey showed that molecular gas was more concentrated to the central kiloparsec in barred spiral galaxies than in their unbarred counterparts. The result provided not only evidence for bar-driven gas transport but also estimates on the mean rate of gas transfer and lower limits to the lifetime of bars. Other lines of evidence for the bar-driven transport of ISM in spiral galaxies are summarized. They are complementary with each other." @default.
- W1799843663 created "2016-06-24" @default.
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- W1799843663 date "1999-10-13" @default.
- W1799843663 modified "2023-09-25" @default.
- W1799843663 title "Bar-driven Transport of Molecular Gas in Spiral Galaxies: Observational Evidence" @default.
- W1799843663 hasPublicationYear "1999" @default.
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