Visible and infrared interferometry before and with the VLT.

Details Visible and infrared interferometry before and with the VLT. Visible and infrared interferometry before and with the VLT.

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991anpcs..16..497p&link_type=abstract

Ann. Phys. (Paris) Colloq., Vol. 16, No. 4, p. 497 - 506

Astronomy and Astrophysics

Astrophysics

Interferometry: Supernovae, Interferometry: Methods Of Observation, Interferometry: Vlt, Infrared Interferometry: Methods Of Observation, Supernova 1987A In Lmc

Scientific paper

After a brief recall of the basic principles of interferometric techniques both at visible and infrared wavelengths, the authors show from a few selected examples the contribution of these techniques in the field of the late stages of stellar evolution; indeed they provide unique constraints to model e.g.: late type evolved stars like Mira variables, protoplanetary nebulae and the supernova SN 1987A, which the authors discuss. As a conclusion, they emphasize the importance of the interferometric capabilities of the future ESO's Very Large Telescope for such astrophysical programs.

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