Optical and ultraviolet study of five stars in the Pleiades open cluster

Details Optical and ultraviolet study of five stars in the Pleiades open cluster Optical and ultraviolet study of five stars in the Pleiades open cluster

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mnras.209..123y&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 209, July 1, 1984, p. 123-137. Research supported by th

Astronomy and Astrophysics

Astronomy

7

Open Clusters, Optical Measurement, Pleiades Cluster, Spaceborne Astronomy, Stellar Spectra, Ultraviolet Astronomy, Absorption Spectra, Abundance, Astronomical Catalogs, Electron Density (Concentration), Gas Density, Interstellar Gas, Iue, Line Spectra

Scientific paper

Optical and ultraviolet observations of five low-reddened stars in the Pleiades open cluster have been obtained with an echelle spectrograph and the IUE satellite. The observed interstellar absorption lines have been analysed with different cloud models to estimate interstellar gas abundances for each line-of-sight. These results have been discussed in the light of current models for diatomic formation.

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