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- W30077382 abstract "The ultraluminous IR galaxy NGC 6240 contains two apparent nuclei visible in the ultraviolet, optical, near infrared and radio regimes. We measured the positions of the nuclei on ground-based U, B, V, R, z and I-band images with reference to astrometric standards. The B, V, R, z positions of the southern nucleus show a systematic trend with wavelength, which is consistent with dust extinction towards the northern nucleus. The southern compact radio source is located at the long-wavelength side of the southern nucleus, while the northern compact radio source is significantly offset (by more than 0″3) to the south of its optical counterpart. We conclude that the 2 cm radio nuclei do not have compact optical counterparts which is probably caused by extinction in the molecular cloud complex between the nuclei" @default.
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- W30077382 date "1993-10-01" @default.
- W30077382 modified "2023-09-24" @default.
- W30077382 title "Extinction and the Wavelength Dependent Positions of the Nuclei of NGC 6240" @default.
- W30077382 hasPublicationYear "1993" @default.
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