High angular resolution observations of the cool giant V Hya

Details High angular resolution observations of the cool giant V Hya High angular resolution observations of the cool giant V Hya

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aas...20718210p&link_type=abstract

American Astronomical Society Meeting 207, #182.10; Bulletin of the American Astronomical Society, Vol. 37, p.1464

Astronomy and Astrophysics

Astronomy

1

Scientific paper

We present the preliminary interferometric observations of the cool giant star V Hya. V Hya, which is known to have mass-loss and to be surrounded by a dust shell,was observed in three narrow-band filters in the H bandpass at the infrared optical telescope array (IOTA), using the IONIC three-telescope beam combiner. The star was also observed at the Keck telescope using an aperture mask. We discuss the results and try to fit simple models to the observed data.

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