Interferometric Studies of Hot Star Disks

Details Interferometric Studies of Hot Star Disks Interferometric Studies of Hot Star Disks

Nov 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..337..211s&link_type=abstract

The Nature and Evolution of Disks Around Hot Stars, ASP Conference Series, Vol. 337, Proceedings of a meeting held 7-9 July 2004

Physics

6

Scientific paper

Interferometry in the visible and in the IR now provides milliarcsecond spatial resolution and thus can be used for studying the circumstellar environment of hot star disks. After a brief introduction on the interferometric technique we will illustrate how the modulus and the phase of the visibility can be used to constrain the physics of hot star disks (Be, B[e]) and stellar surfaces studies through recent results from the GI2T, Keck, MkIII, NPOI, VLA and VLTI interferometers.

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