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- W1645821410 abstract "Although the radio continuum distribution of the HII-region/molecular-cloud complex W33 (peak l = 12°.8, b = -0°.2) resembles a discrete region about 15′ arc in size, the behaviour of the recombination-line velocities (Gardner et al . 1975; Bieging et al . 1978) and molecular-line velocities (OH: Robinson et al . 1970; H 2 CO: Gardner and Whiteoak 1972) has been difficult to interpret in terms of a simple model. There is a difference of opinion as to whether W33 consists of two independent complexes at different distances along the line of sight or a single expanding complex (e.g. Goss et al . 1978)." @default.
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- W1645821410 date "1983-01-01" @default.
- W1645821410 modified "2023-10-09" @default.
- W1645821410 title "The Distribution of 115 GHz CO Towards W33" @default.
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- W1645821410 doi "https://doi.org/10.1017/s1323358000016933" @default.
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