The young pre-main-sequence Ae-type star HR 5999

Details The young pre-main-sequence Ae-type star HR 5999 The young pre-main-sequence Ae-type star HR 5999

Mar 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980iraj...14..122t&link_type=abstract

Irish Astronomical Journal, vol. 14, Mar.-June 1980, p. 122-131; Comments, p. 132.

Astronomy and Astrophysics

Astronomy

1

A Stars, B Stars, Early Stars, Hertzsprung-Russell Diagram, Light Curve, Balmer Series, H Lines, Main Sequence Stars, Stellar Spectra, T Tauri Stars

Scientific paper

The fact that the effective temperature and the gravity of the central star do not change is thought to indicate that the light variation must indeed have something to do with dust grains. This agrees with the infrared observations of Smyth et al. (1979), who showed that HR 5999 has an infrared excess, which at the K passband (2.2 microns) is about 2m.

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