Indicators of star formation: 4000 Angstrom break and Balmer lines

Details Indicators of star formation: 4000 Angstrom break and Balmer lines Indicators of star formation: 4000 Angstrom break and Balmer lines

1997-03-11

arxiv.org/abs/astro-ph/9703067v1

Astronomy and Astrophysics

Astrophysics

5 pages, needs A&A l-aa.sty, accepted for publication in Astronomy & Astrophysics, complete preprint with figures available on

Scientific paper

The behaviour of the 4000 Angstrom break index and of the equivalent width of
the main Balmer lines is investigated a) for a single star as a function of
effective temperature, gravity and metallicity and b) for a single stellar
population as a function of age and metallicity. Consequences for the
interpretation of integrated spectra are presented.

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