Matches in SemOpenAlex for { <https://semopenalex.org/work/W2139146760> ?p ?o ?g. }
- W2139146760 endingPage "926" @default.
- W2139146760 startingPage "911" @default.
- W2139146760 abstract "We present an analysis of ten cool stars (Algol, Capella, Procyon, ϵ Eri, α Cen A&B, UX Ari, AD Leo, YY Gem, and HR 1099) observed with the Low Energy Transmission Grating Spectrometer (LETGS) on board the Chandra X-ray Observatory. This sample contains all cools stars observed with the LETGS presently available to us with integration times sufficiently long to warrant a meaningful spectral analysis. Our sample comprises inactive, moderately active, and hyperactive stars and samples the bulk part of activity levels encountered in coronal X-ray sources. We use the LETGS spectra to carry out density and temperature diagnostics with an emphasis on the H-like and the He-like ions. We find a correlation between line flux ratios of the Lyα and He-like resonance lines with the mean X-ray surface flux. We determine densities using the He-like triplets. For all stars we find no significant deviations from the low-density limit for the ions of Ne, Mg, and Si, while the measured line ratios for the ions of C, N, and O do show evidence for departures from the low-density limit in the active stars, but not in the inactive stars. Best measurements can be made for the O vii triplet where we find significant deviations from the low-density limit for the stars Algol, Procyon, YY Gem, ϵ Eri, and HR 1099. We discuss the influence of radiation fields on the interpretation of the He-like triplet line ratios in the low-Z ions, which is relevant for Algol, and the influence of dielectronic satellite lines, which is relevant for Procyon. For the active stars YY Gem, ϵ Eri, and HR 1099 the low ratios can unambiguously be attributed to high densties in the range 1– cm-3 at O vii temperatures. We find our LETGS spectra to be an extremely useful tool for plasma diagnostics of stellar coronae." @default.
- W2139146760 created "2016-06-24" @default.
- W2139146760 creator A5002377184 @default.
- W2139146760 creator A5031565506 @default.
- W2139146760 creator A5034407636 @default.
- W2139146760 creator A5045660438 @default.
- W2139146760 creator A5056738086 @default.
- W2139146760 creator A5064215797 @default.
- W2139146760 creator A5080924581 @default.
- W2139146760 creator A5084185702 @default.
- W2139146760 date "2002-10-21" @default.
- W2139146760 modified "2023-10-02" @default.
- W2139146760 title "Coronal density diagnostics with Helium-like triplets: CHANDRA–LETGS observations of Algol, Capella, Procyon,<i>ϵ</i> Eri,<i>α</i> Cen A&B, UX Ari, AD Leo, YY Gem, and HR 1099" @default.
- W2139146760 cites W1965545051 @default.
- W2139146760 cites W1973627106 @default.
- W2139146760 cites W1973973816 @default.
- W2139146760 cites W1978467706 @default.
- W2139146760 cites W1982051709 @default.
- W2139146760 cites W1990607376 @default.
- W2139146760 cites W2002845820 @default.
- W2139146760 cites W2011131836 @default.
- W2139146760 cites W2014255857 @default.
- W2139146760 cites W2016466907 @default.
- W2139146760 cites W2020639220 @default.
- W2139146760 cites W2020733834 @default.
- W2139146760 cites W2020749407 @default.
- W2139146760 cites W2035227477 @default.
- W2139146760 cites W2038682297 @default.
- W2139146760 cites W2039001187 @default.
- W2139146760 cites W2058457198 @default.
- W2139146760 cites W2067533103 @default.
- W2139146760 cites W2078622370 @default.
- W2139146760 cites W2085193166 @default.
- W2139146760 cites W2096990639 @default.
- W2139146760 cites W2099207807 @default.
- W2139146760 cites W2150805685 @default.
- W2139146760 cites W2156971590 @default.
- W2139146760 cites W2171332356 @default.
- W2139146760 cites W2949142349 @default.
- W2139146760 cites W3098410852 @default.
- W2139146760 cites W3104523264 @default.
- W2139146760 cites W3104524692 @default.
- W2139146760 cites W4300624548 @default.
- W2139146760 doi "https://doi.org/10.1051/0004-6361:20021146" @default.
- W2139146760 hasPublicationYear "2002" @default.
- W2139146760 type Work @default.
- W2139146760 sameAs 2139146760 @default.
- W2139146760 citedByCount "81" @default.
- W2139146760 countsByYear W21391467602012 @default.
- W2139146760 countsByYear W21391467602013 @default.
- W2139146760 countsByYear W21391467602014 @default.
- W2139146760 countsByYear W21391467602015 @default.
- W2139146760 countsByYear W21391467602016 @default.
- W2139146760 countsByYear W21391467602017 @default.
- W2139146760 countsByYear W21391467602018 @default.
- W2139146760 countsByYear W21391467602019 @default.
- W2139146760 countsByYear W21391467602022 @default.
- W2139146760 countsByYear W21391467602023 @default.
- W2139146760 crossrefType "journal-article" @default.
- W2139146760 hasAuthorship W2139146760A5002377184 @default.
- W2139146760 hasAuthorship W2139146760A5031565506 @default.
- W2139146760 hasAuthorship W2139146760A5034407636 @default.
- W2139146760 hasAuthorship W2139146760A5045660438 @default.
- W2139146760 hasAuthorship W2139146760A5056738086 @default.
- W2139146760 hasAuthorship W2139146760A5064215797 @default.
- W2139146760 hasAuthorship W2139146760A5080924581 @default.
- W2139146760 hasAuthorship W2139146760A5084185702 @default.
- W2139146760 hasBestOaLocation W21391467601 @default.
- W2139146760 hasConcept C121332964 @default.
- W2139146760 hasConcept C1276947 @default.
- W2139146760 hasConcept C145148216 @default.
- W2139146760 hasConcept C150846664 @default.
- W2139146760 hasConcept C184779094 @default.
- W2139146760 hasConcept C191897082 @default.
- W2139146760 hasConcept C192562407 @default.
- W2139146760 hasConcept C198352243 @default.
- W2139146760 hasConcept C2524010 @default.
- W2139146760 hasConcept C33923547 @default.
- W2139146760 hasConcept C44870925 @default.
- W2139146760 hasConcept C4839761 @default.
- W2139146760 hasConcept C546029482 @default.
- W2139146760 hasConcept C62520636 @default.
- W2139146760 hasConcept C68709404 @default.
- W2139146760 hasConceptScore W2139146760C121332964 @default.
- W2139146760 hasConceptScore W2139146760C1276947 @default.
- W2139146760 hasConceptScore W2139146760C145148216 @default.
- W2139146760 hasConceptScore W2139146760C150846664 @default.
- W2139146760 hasConceptScore W2139146760C184779094 @default.
- W2139146760 hasConceptScore W2139146760C191897082 @default.
- W2139146760 hasConceptScore W2139146760C192562407 @default.
- W2139146760 hasConceptScore W2139146760C198352243 @default.
- W2139146760 hasConceptScore W2139146760C2524010 @default.
- W2139146760 hasConceptScore W2139146760C33923547 @default.
- W2139146760 hasConceptScore W2139146760C44870925 @default.
- W2139146760 hasConceptScore W2139146760C4839761 @default.
- W2139146760 hasConceptScore W2139146760C546029482 @default.
- W2139146760 hasConceptScore W2139146760C62520636 @default.
- W2139146760 hasConceptScore W2139146760C68709404 @default.