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- W77370583 abstract "We analyze CO and H 2 absorption lines of the foreground molecular cloud in the Carina nebula. We use HST-STIS (Hubble Space Telescope - Space Telescope Imaging Spectrograph ) & IUE (International Ultraviolet Explorer) INES data to analyze the A-X (v=0→2) absorption band of CO for several hot stars toward the Carina nebula, while 9 stars of them have FUSE (Far Ultraviolet Spectroscopic Explorer) spectra to analyze the (v=0→4) vibrational band in the Lyman series of H 2 . The column densities of CO and H 2 varies in the vicinity of N(CO) ~ 10 13 cm −2 and N(H 2 ) ~ 10 19 cm −2 , respectively. The resultant CO-to-H 2 abundance ratio is about 10 −6 . We investigate the variation of the abundance ratio according to the relative position of the target stars to morphology the molecular cloud in the Carina nebula." @default.
- W77370583 created "2016-06-24" @default.
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- W77370583 date "2004-01-01" @default.
- W77370583 modified "2023-09-24" @default.
- W77370583 title "CO-to-H2 Abundance Ratio of the Foreground Gas of the Carina Nebula" @default.
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- W77370583 doi "https://doi.org/10.1017/s0074180900197438" @default.
- W77370583 hasPublicationYear "2004" @default.
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