Near-Infrared Interferometric Observations of Vega-like Stars

Details Near-Infrared Interferometric Observations of Vega-like Stars Near-Infrared Interferometric Observations of Vega-like Stars

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aas...19913520c&link_type=abstract

American Astronomical Society, 199th AAS Meeting, #135.20; Bulletin of the American Astronomical Society, Vol. 33, p.1508

Astronomy and Astrophysics

Astronomy

Scientific paper

We present H (1.65 μ ; m) and K (2.2 μ ; m) sub-AU angular size measurements for a series of Vega-like stars observed at the Palomar Testbed Interferometer (PTI). These data are part of a long term observational program using PTI to characterize the sub-AU morphology of Vega-like stars. In each case, PTI has resolved the near-infrared emission from these sources. We present the results and discuss the possible emission sources which contribute to measured visibilities.

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