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- W1970430147 abstract "In response to a suggestion by Phillips & Gondhalekar (1981) that hotgas is receding from the I Per OB association with a velocity of ∼30 km s−1, we have examined the IUE high-dispersion spectra of stars in the association for blueshifted lines of interstellar CIV, SiIV and AlIII. As a result, the high-velocity ions are now known to be present in front of at least five stars. Our analysis of the radial velocities of the ions and of the column density ratio N(CIV)/N(SiIV) in the different sight-lines leads to a conclusion similar to that of Phillips & Gondhalekar, namely that the motion of the highly ionized gas is due to a supernova. We believe, however, that the expansion of the HI shell in front of I Per is unrelated and that it is probably due to a recombining HII region within which the supernova event has occurred." @default.
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- W1970430147 date "1985-08-01" @default.
- W1970430147 modified "2023-09-23" @default.
- W1970430147 title "Shock-heated gas in the I Per OB association" @default.
- W1970430147 doi "https://doi.org/10.1093/mnras/215.3.473" @default.
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