Astronomy and Astrophysics – Astrophysics
Scientific paper
2001-06-11
Mon.Not.Roy.Astron.Soc. 327 (2001) 475
Astronomy and Astrophysics
Astrophysics
10 pages, 8 figures, to appear in monthly notices (accepted) (replaced with references)
Scientific paper
10.1046/j.1365-8711.2001.04744.x
We present time resolved K-band infrared spectra of the dwarf nova (DN) IP Peg in early quiescence. The Brackett-gamma and HeI lines in our data show hitherto unseen behaviour, which we term a mirror eclipse, and interpret as an eclipse of the secondary star by an optically thin accretion disc. Mirror eclipses are a direct probe of the structure and physical conditions of accretion discs. For example, on assuming the relevant level populations to be in LTE, we constrain the temperature and density of the optically thin material causing the mirror eclipse to be 10,000 < T < 20,000 K and \rho ~10^-11 g/cm^3 respectively. In order to match our data we find that at least the outermost 20% of the disc (in radius) must be entirely optically thin. Implications for time-dependant disc models are examined.
Dhillon Vik S.
Harlaftis Emilios T.
Littlefair Stuart P.
Marsh Thomas R.
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