Resolving Spiral Shocks of Solar-size Accretion Disks at the Micro-arcsecond Level

Details Resolving Spiral Shocks of Solar-size Accretion Disks at the Micro-arcsecond Level Resolving Spiral Shocks of Solar-size Accretion Disks at the Micro-arcsecond Level

May 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aas...204.0815h&link_type=abstract

American Astronomical Society Meeting 204, #08.15; Bulletin of the American Astronomical Society, Vol. 36, p.982

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Scientific paper

Spiral shocks have been discovered in hot accretion disks in dwarf novae during outbursts, using Doppler maps of HeI and Balmer emission lines. Here, we present the eclipse light curves of these lines and we simulate the parameters that affect dilution of the spiral shock light by the ambient symmetric disk emission. Taking into account the simulations, we reconstruct the maps of the disk and resolve spatially the spiral shocks out of contaminating other emission.

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