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- W1990558304 abstract "We have used the National Radio Astronomy Observatory (NRAO) 12 m telescope to search for CO (J = 1 - 0) emission from the tidal tails of six merging or interacting galaxies. Although these plumes are H I-rich and several contain star forming regions, they are undetected in CO to low levels. The lack of strong CO emission from these plumes in conjunction with the presence of massive star formation is reminiscent of the situation in dwarf irregular galaxies, and the CO/H I limits are consistent with those of dwarfs. The low CO brightness of these plumes may be due either to a low proportion of molecular gas, or to a high N(H2)/I(sub CO) conversion factor." @default.
- W1990558304 created "2016-06-24" @default.
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- W1990558304 date "1994-09-01" @default.
- W1990558304 modified "2023-09-27" @default.
- W1990558304 title "A search for CO (1-0) emission from the tidal structures of interacting and merging galaxies" @default.
- W1990558304 doi "https://doi.org/10.1086/117115" @default.
- W1990558304 hasPublicationYear "1994" @default.
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