Catalog Service: N-band visibilities of V Oph
Description
We present the first multi-epoch N-band spectro-interferometric observations of the carbon-rich Mira variable V Oph using MIDI at the ESO's Very Large Telescope Interferometer. Our aim is to study temporal variations of physical properties of the outer atmosphere and the circumstellar dust shell based on spectrally-dispersed N-band visibilities over the C_2_H_2_ (+HCN) features and the dust emission.
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Publisher: CDSivo://CDS[Pub. ID]
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This resource was registered on: 2007 Jul 14 22:02:35ZThis resource description was last updated on: 2021 Oct 21 00:00:00Z
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Developed with the support of the National Science Foundation under Cooperative Agreement AST0122449 with the Johns Hopkins University The NAVO project is a member of the International Virtual Observatory Alliance
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