SIMBAD references

1997A&A...322..131F - Astronomy and Astrophysics, volume 322, 131-138 (1997/6-1)

The relationship between lithium and activity in disk population main sequence G and K stars.

FAVATA F., MICELA G. and SCIORTINO S.

Abstract (from CDS):

We present determinations of the lithium abundance (through observations of the LiI 6707.8Å line) in a sample of main sequence stars with spectral types ranging from late F down to M0, selected from the sample of nearby stars which have been observed with the Einstein observatory. We show that lithium abundance is correlated with X-ray luminosity for the cooler stars in our sample (4700>Teff>4000), while no correlation is present for the hotter stars. However, the correlation is almost completely driven by a very small number of high lithium, high X-ray luminosity (and thus plausibly very young) cool dwarfs present in the sample. A number of high lithium K dwarfs are present in the survey, and their characteristics and likely age are discussed in detail.

Abstract Copyright:

Journal keyword(s): stars: abundances - stars: late-type

Simbad objects: 64

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