X-ray spectra of 4 cool stars (Sanz-forcada+, 2004)

Details X-ray spectra of 4 cool stars (Sanz-forcada+, 2004) X-ray spectra of 4 cool stars (Sanz-forcada+, 2004)

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004ycat..34160281s&link_type=abstract

VizieR On-line Data Catalog: J/A+A/416/281. Originally published in: 2004A&A...416..281S

Astronomy and Astrophysics

Astrophysics

Stars: Late-Type, X-Ray Sources, Spectroscopy

Scientific paper

These tables include the observed fluxes of the lines identified in the X-ray spectra of four cool stars (Procyon, epsilon Eri, lambda And and V851 Cen). The spectra were taken using different configurations (Chandra/LETG, Chandra/HETG and XMM/RGS). The tables 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.
(4 data files).

Affiliated with

Also associated with

No associations

Rating

X-ray spectra of 4 cool stars (Sanz-forcada+, 2004) does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with X-ray spectra of 4 cool stars (Sanz-forcada+, 2004), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and X-ray spectra of 4 cool stars (Sanz-forcada+, 2004) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1030647