Metal abundances and microturbulence in seven solar-type stars - Spectroscopic data

Details Metal abundances and microturbulence in seven solar-type stars - Spectroscopic data Metal abundances and microturbulence in seven solar-type stars - Spectroscopic data

Mar 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978a%26as...31..297g&link_type=abstract

Astronomy and Astrophysics Supplement Series, vol. 31, Mar. 1978, p. 297-306. Deutsche Forschungsgemeinschaft

Astronomy and Astrophysics

Astrophysics

5

Abundance, Line Spectra, Metals, Spectral Line Width, Stellar Spectra, Tables (Data), Balmer Series, Graphs (Charts)

Scientific paper

Basic spectroscopic data for the analyses of seven solar-type stars are
presented, including the computational results for individual spectral
lines in the wavelength region from 4400 to 6800 A. Line strengths are
compared with previous observations by other authors.

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