Relative intensities of intercombination lines in ultraviolet spectra of T Tauri stars

Details Relative intensities of intercombination lines in ultraviolet spectra of T Tauri stars Relative intensities of intercombination lines in ultraviolet spectra of T Tauri stars

Nov 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998astl...24..748l&link_type=abstract

Astronomy Letters, Volume 24, Issue 6, November 1998, pp.748-752; Pis'ma v Astronomicheskii Zhurnal, Vol. 24, p. 862

Astronomy and Astrophysics

Astronomy

6

Scientific paper

Using the accretion shock wave model (Lamzin 1998), we calculate the relative intensities of the strongest intercombination lines in the range 1200-2000 Angstroms. We make a qualitative comparison of theoretical spectra with IUE low-resolution (~=6 Angstroms) spectra of T Tauri stars. We predict that several intercombination lines can be identified in spectroscopic observations of young stars with the Hubble Space Telescope and used for a quantitative comparison with the calculations.

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