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- W1671557118 abstract "The planetary nebula Hb 12 has recently been observed at infrared (Aitken et al., 1979) and radio (Purton et al., 1982) wavelengths. The detection of a silicate emission feature in the 8-13 μm region suggests that the nebula is oxygen rich. A high emission measure is derived from the radio spectrum, implying a high intrinsic density." @default.
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- W1671557118 date "1983-01-01" @default.
- W1671557118 modified "2023-10-17" @default.
- W1671557118 title "Physical Conditions in the Planetary Nebula Hb 12" @default.
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- W1671557118 doi "https://doi.org/10.1017/s0074180900094213" @default.
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