Spectral Evolution and Line Strength Indices in the UV

Details Spectral Evolution and Line Strength Indices in the UV Spectral Evolution and Line Strength Indices in the UV

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009nqsa.conf..283b&link_type=abstract

New Quests in Stellar Astrophysics. II. Ultraviolet Properties of Evolved Stellar Populations, Proceedings of the International

Astronomy and Astrophysics

Astrophysics

Scientific paper

The Hubble New Generation Spectral Library (HNGSL) provides a unique opportunity to explore evolutionary population synthesis models in the UV. The library contains spectra for a few hundred stars with fundamental parameters known from analysis of the visual spectrum. The spectra cover fully the wavelength range from 1700 Å to 10,200 Å with spectral resolution close to 5 Å, providing excellent coverage of the near-UV and the range from 9000 Å to 10,200 Å.

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