Spectroscopic behaviour of the Herbig Be star HD200775 around its maximum activity in 1997

UNCG Author/Contributor (non-UNCG co-authors, if there are any, appear on document)

Anatoly S. Miroshnichenko, Professor (Creator)

Institution

The University of North Carolina at Greensboro (UNCG )

Web Site: http://library.uncg.edu/

Abstract: We present the results of high-resolution spectroscopic observations of the pre-main-sequence (PMS) Herbig Be star HD200775 obtained between August 1994 and December 1999. The behaviour of H, H and He i before, during, and after the last high-activity event of the object in 1997 is studied. Acomplex picture of the circumstellar evolution in this period is discussed. It is concluded that the results of observations can be interpreted in the framework of a model with a variable stellar wind originating from the star. We emphasize the importance of coordinated high-resolution spectroscopic observations for further understanding the star’s behaviour.

Spectroscopic behaviour of the Herbig Be star HD200775 around its maximum activity in 1997
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Created on 7/1/2000
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Additional Information

Publication

(2000) Miroshnichenko, A.S et al. Spectroscopic behaviour of the Herbig Be star HD 200775 around its maximum activity in 1997. Astronomy & Astrophysics 359, 299-305

Language: English

Date: 2000

Keywords

Techniques: spectroscopic, Stars: circumstellar matter, Stars: individual: HD 200775, Stars: pre-main sequence

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