Interferometric Observations of Nova Aql 2005

Details Interferometric Observations of Nova Aql 2005 Interferometric Observations of Nova Aql 2005

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aas...20710408l&link_type=abstract

American Astronomical Society Meeting 207, #104.08; Bulletin of the American Astronomical Society, Vol. 37, p.1335

Astronomy and Astrophysics

Astronomy

1

Scientific paper

We report on observations of Nova Aql 2005 (V1663 Aql) using the Palomar Testbed Interferometer. Near-infrared observations of the nova were initiated approximately 9 days after peak luminosity and continued for 10 days. Using the three available baselines we resolved the milliarcsecond-scale emission and measured the shape and angular size of the nova photosphere as a function of time. These observations can be combined with radial-velocity information to produce a geometric distance (and hence luminosity) estimate.

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