Current Models of FUORs

Details Current Models of FUORs Current Models of FUORs

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007jena.confe..24l&link_type=abstract

"JENAM-2007, "Our non-stable Universe", held 20-25 August 2007 in Yerevan, Armenia. Abstract book, p. 24-24"

Computer Science

Scientific paper

We consider problems in interpretation of FUORs observations in the frame of two competitive theoretical models: accretion α-disc and rapidly rotating supergiant. We argue that advective accretion disk model can solve these problems. The height of such disk increases inward starting from r ~ 10^12 cm, reaches the maximum value at r ~ 3R* and then decreases, such as disk's innermost regions have a cone-like shape. The model is a compromise between models of thin disk and supergiant: it is an accretion model but observational manifestations of such disk is very similar to G0-supergiant.

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