The Herbig Ae/Be Star V586 Ori

Details The Herbig Ae/Be Star V586 Ori The Herbig Ae/Be Star V586 Ori

Jan 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004ap.....47....1c&link_type=abstract

Astrophysics (English translation of Astrofizika), v. 47, Issue 1, p. 1-10 (2004).

Astronomy and Astrophysics

Astrophysics

Stars Photometry - Individual Stars - V586 Ori

Scientific paper

Studies of the Herbig Ae/Be star V586 Ori based on photoelectric observations in the Strömgren system are reported. It is found that as the brightness decreases, the Balmer discontinuity index initially increases and then begins to drop. As the star fades, the index decreases. We have previously found similar variations in the indices and C for UX Ori, RR Tau, and V351 Ori. It is shown that V586 Ori has the characteristics of a shell-star.

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