X-ray spectrum of SV Cam (Sanz-Forcada+, 2006)

Details X-ray spectrum of SV Cam (Sanz-Forcada+, 2006) X-ray spectrum of SV Cam (Sanz-Forcada+, 2006)

Nov 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ycat..34450673s&link_type=abstract

VizieR On-line Data Catalog: J/A+A/445/673. Originally published in: 2006A&A...445..673S

Astronomy and Astrophysics

Astrophysics

Stars: Variable, Spectroscopy, X-Ray Sources

Scientific paper

This table includes the observed fluxes of the lines identified in the X-ray spectrum (XMM/RGS) of SV Cam. The table list the observed fluxes at Earth, and a comparison with the fluxes predicted for a given thermal coronal structure (the Emission Measure Distribution, EMD), the emissivities provided by the Astrophysical Plasma Emission Model (APED), and column density of absorbing material in the interstellar medium towards the star. A list of the most important (at least a 5% of the flux predicted for the line) blends that have been considered for each line is included.
(1 data file).

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