Detection of an infrared companion to Haro 6-10

Details Detection of an infrared companion to Haro 6-10 Detection of an infrared companion to Haro 6-10

Jul 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...342l..39l&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 342, July 1, 1989, p. L39-L42.

Astronomy and Astrophysics

Astronomy

59

Companion Stars, Herbig-Haro Objects, Infrared Sources (Astronomy), Pre-Main Sequence Stars, Speckle Interferometry, Binary Stars, Near Infrared Radiation, Star Formation, Stellar Mass

Scientific paper

Near-IR speckle observations showed the IR source of Haro 6-10 to be double with the two components separated by 1.2 arcsecs at position angle 355 deg. At wavelengths shorter than 3.8 microns, the southern component dominates, while most of the IR radiation longward of 4 microns arises from the extremely red northern component. Both components are unresolved in north-south scans. It is suggested that they are stellar and form a young low-mass binary. The detected IR companion is probably similar to those found earlier for a few T Tau stars.

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