The remarkable Herbig Ae star V351 Ori.

Details The remarkable Herbig Ae star V351 Ori. The remarkable Herbig Ae star V351 Ori.

Oct 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996nascp3339...33v&link_type=abstract

Scientific conference: From stardust to planetesimals, p. 33 - 36

Physics

Photometry: Herbig Ae-Be Stars, Herbig Ae-Be Stars: Stellar Evolution, Circumstellar Dust: Herbig Ae-Be Stars

Scientific paper

The photometric behaviour of the Herbig Ae star V351 Ori was investigated combining data from the literature with new photometry. It is shown that this object changed from a Herbig Ae star with strong photometric variations, due to extinction by circumstellar dust clouds, to that of an almost non-variable star. A provisional model to explain V351 Ori's behaviour, in which it is assumed that a temporarily strong accretion of matter onto the star took place, is proposed.

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