Dusty disk wind in young binary systems viewed pole-on

Details Dusty disk wind in young binary systems viewed pole-on Dusty disk wind in young binary systems viewed pole-on

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ap.....51..218t&link_type=abstract

Astrophysics, Volume 51, Issue 2, pp.218-225

Astronomy and Astrophysics

Astrophysics

Stars, Binaries, Dust

Scientific paper

A model of a young binary system with companions of unequal mass whose orbital plane is inclined at a large angle to the line of sight is examined. The system components are assumed to accrete matter from the remains of the protostellar cloud. It is found that eclipsing of the primary component by the disk wind of the secondary can be observed when the plane of the orbit is inclined at a large angle to the line of sight or even when the binary system is observed pole-on.

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