FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3100898622> ?p ?o ?g. }

• W3100898622 endingPage "981" @default.
• W3100898622 startingPage "965" @default.
• W3100898622 abstract "We present an analysis of our Chandra Low Energy Transmission Grating Spectrometer (LETGS) observation of the quasar MR 2251–178. The warm absorber of MR 2251–178 is well described by a hydrogen column density NH ≈ 2 × 1021 cm−2 and an ionization parameter log (ξ ) ≈ 0.6. We find in the spectrum weak evidence for narrow absorption lines from carbon and nitrogen which indicate that the ionized material is in outflow. We note changes (in time) of the absorption structure in the band 0.6-1 keV (around the unresolved transition arrays [UTAs] plus the O VII and O VIII K edges) at different periods of the observation. We measure a 0.1-2 keV flux of 2.58 × 10−11 ergs cm−2 s−1. This flux implies that the nuclear source of MR 2251–178 is in a relatively low state. No significant variability is seen in the light curve. We do not find evidence for extra cold material in the line of sight, and set an upper limit of NH ≈ 1.2 × 1020 cm−2. The X-ray spectrum does not appear to show evidence for dusty material, although an upper limit in the neutral carbon and oxygen column densities can only be set to cm−2 and cm−2, respectively." @default.
• W3100898622 created "2020-11-23" @default.
• W3100898622 creator A5031796723 @default.
• W3100898622 creator A5047273464 @default.
• W3100898622 creator A5083366614 @default.
• W3100898622 creator A5084185702 @default.
• W3100898622 date "2008-07-10" @default.
• W3100898622 modified "2023-10-16" @default.
• W3100898622 title "<i>Chandra</i>LETGS Spectroscopy of the Quasar MR 2251−178 and Its Warm Absorber" @default.
• W3100898622 cites W1971541527 @default.
• W3100898622 cites W1973164872 @default.
• W3100898622 cites W1977457396 @default.
• W3100898622 cites W1986682069 @default.
• W3100898622 cites W2000369505 @default.
• W3100898622 cites W2007319080 @default.
• W3100898622 cites W2013742280 @default.
• W3100898622 cites W2015411431 @default.
• W3100898622 cites W2017396100 @default.
• W3100898622 cites W2031680507 @default.
• W3100898622 cites W2036437339 @default.
• W3100898622 cites W2038787622 @default.
• W3100898622 cites W2039777668 @default.
• W3100898622 cites W2048062091 @default.
• W3100898622 cites W2049276365 @default.
• W3100898622 cites W2051490449 @default.
• W3100898622 cites W2054169395 @default.
• W3100898622 cites W2073155743 @default.
• W3100898622 cites W2079652885 @default.
• W3100898622 cites W2091403098 @default.
• W3100898622 cites W2094714727 @default.
• W3100898622 cites W2109118639 @default.
• W3100898622 cites W2111818748 @default.
• W3100898622 cites W2117800225 @default.
• W3100898622 cites W2147074747 @default.
• W3100898622 cites W2158478093 @default.
• W3100898622 cites W2169522826 @default.
• W3100898622 cites W2952760878 @default.
• W3100898622 cites W3100064991 @default.
• W3100898622 cites W3100921344 @default.
• W3100898622 cites W3102090152 @default.
• W3100898622 cites W3104819605 @default.
• W3100898622 cites W3104820388 @default.
• W3100898622 cites W3105853033 @default.
• W3100898622 doi "https://doi.org/10.1086/587949" @default.
• W3100898622 hasPublicationYear "2008" @default.
• W3100898622 type Work @default.
• W3100898622 sameAs 3100898622 @default.
• W3100898622 citedByCount "13" @default.
• W3100898622 countsByYear W31008986222013 @default.
• W3100898622 countsByYear W31008986222014 @default.
• W3100898622 countsByYear W31008986222015 @default.
• W3100898622 countsByYear W31008986222016 @default.
• W3100898622 countsByYear W31008986222017 @default.
• W3100898622 countsByYear W31008986222021 @default.
• W3100898622 crossrefType "journal-article" @default.
• W3100898622 hasAuthorship W3100898622A5031796723 @default.
• W3100898622 hasAuthorship W3100898622A5047273464 @default.
• W3100898622 hasAuthorship W3100898622A5083366614 @default.
• W3100898622 hasAuthorship W3100898622A5084185702 @default.
• W3100898622 hasBestOaLocation W31008986221 @default.
• W3100898622 hasConcept C119824511 @default.
• W3100898622 hasConcept C120665830 @default.
• W3100898622 hasConcept C121332964 @default.
• W3100898622 hasConcept C125287762 @default.
• W3100898622 hasConcept C1276947 @default.
• W3100898622 hasConcept C135041427 @default.
• W3100898622 hasConcept C145148216 @default.
• W3100898622 hasConcept C184779094 @default.
• W3100898622 hasConcept C191897082 @default.
• W3100898622 hasConcept C192562407 @default.
• W3100898622 hasConcept C198291218 @default.
• W3100898622 hasConcept C198352243 @default.
• W3100898622 hasConcept C2524010 @default.
• W3100898622 hasConcept C2780928442 @default.
• W3100898622 hasConcept C32891209 @default.
• W3100898622 hasConcept C33923547 @default.
• W3100898622 hasConcept C44870925 @default.
• W3100898622 hasConcept C4839761 @default.
• W3100898622 hasConcept C62520636 @default.
• W3100898622 hasConcept C68709404 @default.
• W3100898622 hasConcept C98444146 @default.
• W3100898622 hasConceptScore W3100898622C119824511 @default.
• W3100898622 hasConceptScore W3100898622C120665830 @default.
• W3100898622 hasConceptScore W3100898622C121332964 @default.
• W3100898622 hasConceptScore W3100898622C125287762 @default.
• W3100898622 hasConceptScore W3100898622C1276947 @default.
• W3100898622 hasConceptScore W3100898622C135041427 @default.
• W3100898622 hasConceptScore W3100898622C145148216 @default.
• W3100898622 hasConceptScore W3100898622C184779094 @default.
• W3100898622 hasConceptScore W3100898622C191897082 @default.
• W3100898622 hasConceptScore W3100898622C192562407 @default.
• W3100898622 hasConceptScore W3100898622C198291218 @default.
• W3100898622 hasConceptScore W3100898622C198352243 @default.
• W3100898622 hasConceptScore W3100898622C2524010 @default.
• W3100898622 hasConceptScore W3100898622C2780928442 @default.
• W3100898622 hasConceptScore W3100898622C32891209 @default.
• W3100898622 hasConceptScore W3100898622C33923547 @default.
• W3100898622 hasConceptScore W3100898622C44870925 @default.

• next