A thin shell of ionized gas as the explanation for infrared excess among classical Cepheids

V. Hocdé; N. Nardetto; E. Lagadec; G. Niccolini; A. Domiciano de Souza; A. Mérand; P. Kervella; A. Gallenne; M. Marengo; B. Trahin; W. Gieren; G. Pietrzyński; S. Borgniet; L. Breuval; B. Javanmardi

doi:10.1051/0004-6361/201935848

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Volume 633 (January 2020)

A&A, 633 (2020) A47

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Table 9

IR excess from the ionized shell models in various bands of the JWST.

	Δ F070W	Δ F200W	Δ F560W	Δ F1000W
RS Pup	0.110	0.009	−0.074	−0.100
ζ Gem	0.090	0.016	−0.029	−0.034
η Aql	0.220	0.030	−0.038	−0.037
V Cen	0.069	0.004	−0.071	−0.101
SU Cyg	0.063	0.001	−0.071	−0.105

Notes. Wide filters F070W, F200W, F560W and F1000W centered respectively on 0.70, 2, 5.6 and 10 μm are presented. Values are given in magnitudes.

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