The Pre Main Sequence Shell Star HR5999 Unveiled

Details The Pre Main Sequence Shell Star HR5999 Unveiled The Pre Main Sequence Shell Star HR5999 Unveiled

Mar 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981msngr..23...25t&link_type=abstract

The Messenger, No.23, P. 25, 1981

Physics

Scientific paper

The star HR 5999 is embedded in a dusty gaseous nebulosity and is surrounded by more than 10 faint T Tauri stars. From these facts and from studies so far made of the physical properties of HR 5999, we strongly believe that it is a very young pre-main-sequence object; it varies irregularly due most probably to changes in the properties of dust grains embedded in its circumstellar gas shell.

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