J. P. Swings scite author profile

The majority of symbiotic and VV Cephei stars have near infrared continua closely resembling those of late-type stars. Evidence for weak infrared excesses has been found in the three stars RY Set, W Cep, and U Lac. RX Pup and V1016 Cyg exhibit very prominent infrared excesses which are attributable to thermal radiation from circumstellar dust.The "Rep" star MWC 56, whose spectrum shows Fen and [Fen] emission lines in the blue, possesses the absorption lines of a G or K component in the red. No substantial infrared excess is present.

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The spectrum of the Antares nebula

Swings¹,

Preston²

1978

ApJ

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J. P. Swings

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The spectrum of the Antares nebula

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