On the emission-line intensities and light-curve characteristics of Orion-population stars

Details On the emission-line intensities and light-curve characteristics of Orion-population stars On the emission-line intensities and light-curve characteristics of Orion-population stars

May 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980mnras.191..321w&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 191, May 1980, p. 321-324.

Astronomy and Astrophysics

Astronomy

6

Emission Spectra, Light Curve, Stellar Luminosity, Stellar Spectra, T Tauri Stars, Astronomical Catalogs, Classifications, H Alpha Line, Statistical Analysis

Scientific paper

The Orion-population stars listed in the Herbig-Rao catalogue show a strong correlation between Parenago light-curve classification and emission-line intensities in a sense different from that expected from the behaviour of individual stars. In addition, the range in brightness variability of these stars appears to be independent of emission-line strength and lightcurve classification.

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