The chemical composition of the galactic H II regions M8 and M17. A revision based on deep VLT echelle spectrophotometry5

We present new echelle spectrophotometry of the Galactic H II regions M8 and M17. The data have been taken with the VLT UVES echelle spectrograph in the 3100 to 10400 Å range. We have measured the intensities of 375 and 260 emission lines in M8 and M17 respectively, increasing significatively the nu...

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Bibliographic Details
Main Author: Monica Rodriguez
Format: info:eu-repo/semantics/article
Published: Revista mexicana de astronomía y astrofísica 2007
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