Disks around pre-main-sequence binary systems - The case of Haro 6-10

Details Disks around pre-main-sequence binary systems - The case of Haro 6-10 Disks around pre-main-sequence binary systems - The case of Haro 6-10

Sep 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993apj...414l.117m&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 414, no. 2, p. L117-L120.

Astronomy and Astrophysics

Astronomy

26

Binary Stars, Pre-Main Sequence Stars, Stellar Envelopes, Astronomical Interferometry, Astronomical Polarimetry, Infrared Astronomy, Speckle Interferometry, Star Formation

Scientific paper

Subarcsecond KLM images of the premain-sequence star Haro 6-10 obtained with the CIRCUS IR camera attached to the Canada-France-Hawaii Telescope are presented. They are the first images where both components of the Haro 6-10 binary system are resolved. We confirm the results by Leinert and Haas (1989), obtained from speckle interferometry, that the projected separation of the two stars is 1.25 arcsec at position angle 356 deg. We also present new polarization measurement and models that suggest the presence of a flat circumbinary envelope (possibly a disk) associated with the system.

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