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- W68558796 abstract "Dense gas in molecular cloud cores is essential in researches of extragalactic star formation (e.g. Solomon, Downes, and Radford). To determine the physical relations between star-forming regions and dense gas, we have observed CS ( J =3→2) in starburst galaxies M 82 and NGC253. The J = 3 level of CS is 14.1 K and the critical density for excitation is 4 × 10 5 cm −3 ." @default.
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- W68558796 date "1994-01-01" @default.
- W68558796 modified "2023-10-18" @default.
- W68558796 title "CS(3-2) in Nearby Starburst Galaxies M82 and NGC253" @default.
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- W68558796 doi "https://doi.org/10.1017/s0252921100019928" @default.
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