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- W151988082 abstract "The physical condition of molecular gas in galaxies is traced by multitransition 12CO and 13CO intensities. We report on a large survey of spiral galaxy centers. In most of these galaxies, significant concentrations of molecular gas occur within a kiloparsec from their nucleus. This gas consists of at least two components: one is hot and relatively tenuous, the other is dense and relatively cool. Much of the gas mass is in the hot component. As the CO-to-H2 conversion factor X is much lower in galaxy centers than in the Milky Way disk, total molecular hydrogen masses are typically an order of magnitude lower than estimated by using the standard value of X." @default.
- W151988082 created "2016-06-24" @default.
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- W151988082 date "2009-01-01" @default.
- W151988082 modified "2023-09-26" @default.
- W151988082 title "Physical conditions of molecular gas in spiral galaxy centers" @default.
- W151988082 hasPublicationYear "2009" @default.
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