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- W2483364926 abstract "Narrow OH emission lines at 1667 MHz, apparently from a Class I source, have been observed near the reflection nebula NGC 2071. The region contains many T Tauri stars. OH emission corresponding to the dust cloud north and east of NGC 2024 is also seen. At 1720 MHz the dust cloud component appears in absorption; presumably the isotropic 2.7 K cosmic background is being absorbed." @default.
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- W2483364926 date "1974-01-01" @default.
- W2483364926 modified "2023-09-26" @default.
- W2483364926 title "Oh Observations Near the Reflection Nebulae Ngc 2068 and Ngc 2071" @default.
- W2483364926 doi "https://doi.org/10.1017/s0074180900026590" @default.
- W2483364926 hasPublicationYear "1974" @default.
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