Astronomy and Astrophysics, volume 507, 317-326 (2009/11-3)
A binary engine fuelling HD 87643's complex circumstellar environment. Determined using AMBER/VLTI imaging.
MILLOUR F., CHESNEAU O., BORGES FERNANDES M., MEILLAND A., MARS G., BENOIST C., THIEBAUT E., STEE P., HOFMANN K.-H., BARON F., YOUNG J., BENDJOYA P., CARCIOFI A., DOMICIANO DE SOUZA A., DRIEBE T., JANKOV S., KERVELLA P., PETROV R.G., ROBBE-DUBOIS S., VAKILI F., WATERS L.B.F.M. and WEIGELT G.
Abstract (from CDS):
The star HD87643, exhibiting the ``B[e] phenomenon'', has one of the most extreme infrared excesses for this object class. It harbours a large amount of both hot and cold dust, and is surrounded by an extended reflection nebula. One of our major goals was to investigate the presence of a companion in HD87643. In addition, the presence of close dusty material was tested through a combination of multi-wavelength high spatial resolution observations. We observed HD87643 with high spatial resolution techniques, using the near-IR AMBER/VLTI interferometer with baselines ranging from 60m to 130m and the mid-IR MIDI/VLTI interferometer with baselines ranging from 25m to 65m. These observations are complemented by NACO/VLT adaptive-optics-corrected images in the K and L-bands, and ESO-2.2m optical Wide-Field Imager large-scale images in the B, V and R-bands. We report the direct detection of a companion to HD87643 by means of image synthesis using the AMBER/VLTI instrument. The presence of the companion is confirmed by the MIDI and NACO data, although with a lower confidence. The companion is separated by ∼34mas with a roughly north-south orientation. The period must be large (several tens of years) and hence the orbital parameters are not determined yet. Binarity with high eccentricity might be the key to interpreting the extreme characteristics of this system, namely a dusty circumstellar envelope around the primary, a compact dust nebulosity around the binary system and a complex extended nebula suggesting past violent ejections.
techniques: high angular resolution - techniques: interferometric - stars: emission-line, Be - binaries: close - circumstellar matter - stars: individual: HD 87643
Fig. 6: [MCB2009] AN (Nos A1-A7, B1-B4).
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