Using Data of VO to Examine X-Ray Astrophysical Sources and Their Applying to the Theoretical Investigations

Details Using Data of VO to Examine X-Ray Astrophysical Sources and Their Applying to the Theoretical Investigations Using Data of VO to Examine X-Ray Astrophysical Sources and Their Applying to the Theoretical Investigations

Apr 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006vopc.conf..400a&link_type=abstract

Virtual Observatory: Plate Content Digitization, Archive Mining and Image Sequence Processing, iAstro workshop, Sofia, Bulgaria,

Astronomy and Astrophysics

Astrophysics

Scientific paper

In this paper we discuss how Virtual Observatories can help us in our investigations pointed to X-ray astrophysical objects in particular close binaries with accretion flows. It is known that emission from accretion discs irradiates by X-rays, which spectrum gives properties of the studying object. Due to analysis of the VO data we may compare the observational results with our theoretical research. We explain here, the necessity of expanding further VO toward X-ray observational data.

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