Interferometric Observations of V1663 Aquilae (Nova Aql 2005)
Astrophysics
2009-11-13 v1
Abstract
We have resolved the classical nova V1663 Aql using long-baseline near-IR interferometry covering the period from 5--18 days after peak brightness. We directly measure the shape and size of the fireball, which we find to be asymmetric. In addition we measure an apparent expansion rate of 0.21 +/- 0.03 mas/day. Assuming a linear expansion model we infer a time of initial outburst approximately 4 days prior to peak brightness. When combined with published spectroscopic expansion velocities our angular expansion rate implies a distance of 8.9 +/- 3.6 kpc. This distance measurement is independent of, but consistent with, determinations made using widely available photometric relations for novae.
Keywords
Cite
@article{arxiv.0710.2128,
title = {Interferometric Observations of V1663 Aquilae (Nova Aql 2005)},
author = {B. F. Lane and A. Retter and J. A. Eisner and Matthew W. Muterspaugh and R. R. Thompson and J. L. Sokoloski},
journal= {arXiv preprint arXiv:0710.2128},
year = {2009}
}
Comments
6 Pages, Accepted for publication in ApJ