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- W3122210395 abstract "Reanalysis of the NIR spectrum of the star-formation object WL 16 indicates that the observed infrared CO emission has a high optical depth, creating a CO emission continuum feature. A new extinction value A(v) = 40 places the Brackett gamma emission within the normal range for low-luminosity line excess sources. The observations are consistent with a spherical cooling outflow with the infrared CO and hydrogen emission arising from physically separate regions. Other geometries are not excluded by the observations. 17 refs." @default.
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- W3122210395 date "1988-09-01" @default.
- W3122210395 modified "2023-09-27" @default.
- W3122210395 title "Optically Thick Infrared CO Emission in WL 16" @default.
- W3122210395 hasPublicationYear "1988" @default.
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