An interferometric study of the post-AGB binary 89 Herculis - I. Spatially resolving the continuum circumstellar environment at optical and near-IR wavelengths with the VLTI, NPOI, IOTA, PTI, and the CHARA Array

M. Hillen; T. Verhoelst; H. Van Winckel; O. Chesneau; C. A. Hummel; J. D. Monnier; C. Farrington; C. Tycner; D. Mourard; T. ten Brummelaar; D. P. K. Banerjee; R. T. Zavala

doi:10.1051/0004-6361/201321616

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Volume 559 (November 2013)

A&A, 559 (2013) A111

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Table 5

Fluxes used in the “stellar SED” fit.

Photometric filter	Total	Stellar	Error

JOHNSON.V	5.45^a	6.00	0.15
JOHNSON.R	5.13	5.68	0.12
2MASS.H^b	4.21	4.86	0.11
2MASS.Ks^b	3.41	4.92	0.1
JOHNSON.H	4.39	5.04	0.12
JOHNSON.K	3.35	4.85	0.12

Notes. For each filter, both the total flux and the stellar flux, i.e. the total flux corrected with the stellar flux fractions of Table 4, are listed.

^(a)

Average of AAVSO light curve over 2011–2012;

^(b)

Mt. Abu measurements.

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