Multicolour photometry and the dust shell of HR 5999

Details Multicolour photometry and the dust shell of HR 5999 Multicolour photometry and the dust shell of HR 5999

Apr 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979mnras.187p..29s&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 187, Apr. 1979, p. 29P-33P.

Astronomy and Astrophysics

Astronomy

11

Astronomical Photometry, Colorimetry, Cosmic Dust, Stellar Envelopes, Variable Stars, Companion Stars, Stellar Mass Ejection, Stellar Models, Tables (Data)

Scientific paper

Infrared observations are presented which reinforce the conclusion reached from optical data that the variability of HR 5999, sometimes being misidentified as HR 6000, is due to ejected dust grains. A simple model is proposed for the existing dust shell. This simple model fits the colors reasonably well. Visible and IR observations planned at a number of observatories for 1978 are expected to give a much more complete picture of this interesting system.

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