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- W2051230682 abstract "Brackett-alpha and Brackett-gamma lines are used to study star formation in the external, interacting galaxies NGC 5195, IC 4553, and the NGC 3690 + IC 694 system. The 10 micron continuum flux in IC 694 appears to be higher than that expected from Galactic type H II regions. Upper limits to the Brackett line emission in NGC 5195 and IC 4553 indicate that in these sources, the infrared continua are poorly correlated with the amount of observed ionized gas. In NGC 5195, the 10 micron excess is probably due to abnormally hot dust. In IC 4553, the intense far-infrared continuum suggests that either there is unusually high obscuration of the star forming regions, or that the young OB stars may produce only a small portion of the infrared luminosity. 27 references." @default.
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- W2051230682 date "1986-10-01" @default.
- W2051230682 modified "2023-10-14" @default.
- W2051230682 title "Infrared spectroscopy of star formation in interacting galaxies" @default.
- W2051230682 doi "https://doi.org/10.1086/164578" @default.
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