The dusty disk winds in young binary systems with the low-mass secondary components

Details The dusty disk winds in young binary systems with the low-mass secondary components The dusty disk winds in young binary systems with the low-mass secondary components

Oct 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003esasp.539..429g&link_type=abstract

In: Proceedings of the Conference on Towards Other Earths: DARWIN/TPF and the Search for Extrasolar Terrestrial Planets, 22-25 A

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Young Binaries, Low-Mass Companions, Disk Winds

Scientific paper

We consider the possible observational effects produced by the dusty disk winds in the young binary systems with the low-mass secondary components. One of them is the photometric effect caused by the eclipses of the main component by the dusty disk wind of the secondary. Another one is connected with the formation of the asymmetric dust and gas common envelopes and lobes. Their scattered and thermal radiation can be the source of the cyclic variations of the linear polarization and that of the infrared radiation of young stars. The calculations show that these effects can be also observed if the low-mass companion is the giant protoplanet in the stage of intensive mass accretion.

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