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- W2080285004 abstract "Three infrared and radio sources in NGC 7538 have been observed with 1% spectral and 5-arcsec spatial resolution. The very small southern source shows a deep silicate absorption feature at 9.7 microns, while the northern extended source shows little or no silicate absorption, but has a 12.8-micron emission line from Ne II. The data imply that the compact source has a gas-to-dust ratio of 75 inside the ionized region. The extended source only 10 arcsec away has a gas-to-dust ratio implied by the 10-micron data alone of 30,000, but the true ratio must be much lower to account for published 20-micron measurements." @default.
- W2080285004 created "2016-06-24" @default.
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- W2080285004 date "1976-06-01" @default.
- W2080285004 modified "2023-09-27" @default.
- W2080285004 title "8 to 13 micron spectrophotometry of compact sources in NGC 7538" @default.
- W2080285004 doi "https://doi.org/10.1086/154433" @default.
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