On the Ionization Structure of Circumstellar Disks Around Be Type Stars

Details On the Ionization Structure of Circumstellar Disks Around Be Type Stars On the Ionization Structure of Circumstellar Disks Around Be Type Stars

Jun 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ap%26ss.263..243t&link_type=abstract

Astrophysics and Space Science, v. 263, Issue 1/4, p. 243-246 (1998).

Astronomy and Astrophysics

Astrophysics

Scientific paper

We present some insight on the ionization structure of the circumstellar disks around Be type stars based on the study of Balmer decrements for absorption-corrected emission lines. Owing to this analysis, three different ionization zones in the envelope are proposed: the inner one, completely ionized, of about ˜ 5R*, an intermediate recombination zone extending up to ˜ [10 - 20]R*, and an outer extended zone of neutral H.

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