FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3100802265> ?p ?o ?g. }

• W3100802265 endingPage "117" @default.
• W3100802265 startingPage "117" @default.
• W3100802265 abstract "Like other young stellar objects (YSOs), FU Ori-type stars have been detected as strong X-ray emitters. However, little is known about how the outbursts of these stars affect their X-ray properties. We assemble available X-ray data from XMM-Newton and Chandra observations of 16 FU Ori stars, including a new XMM-Newton observation of Gaia 17bpi during its optical rise phase. Of these stars, six were detected at least once, while 10 were non-detections, for which we calculate upper limits on intrinsic X-ray luminosity (LX) as a function of plasma temperature (kT) and column density (NH). The detected FU Ori stars tend to be more X-ray luminous than is typical for non-outbursting YSOs, based on comparison to a sample of low-mass stars in the Orion Nebula Cluster. FU Ori stars with high LX have been observed both at the onset of their outbursts and decades later. We use the Kaplan–Meier estimator to investigate whether the higher X-ray luminosities for FU Ori stars are characteristic or a result of selection effects, and we find the difference to be statistically significant (p < 0.01) even when non-detections are taken into account. The additional X-ray luminosity of FU Ori stars relative to non-outbursting YSOs cannot be explained by accretion shocks, given the high observed plasma temperatures. This suggests that, for many FU Ori stars, either (1) the outburst leads to a restructuring of the magnetosphere in a way that enhances X-ray emission, or (2) FU Ori outbursts are more likely to occur among YSOs with the highest quiescent X-ray luminosity." @default.
• W3100802265 created "2020-11-23" @default.
• W3100802265 creator A5013321503 @default.
• W3100802265 creator A5021958638 @default.
• W3100802265 date "2019-09-26" @default.
• W3100802265 modified "2023-10-18" @default.
• W3100802265 title "A Comparison of the X-Ray Properties of FU Ori-type Stars to Generic Young Stellar Objects" @default.
• W3100802265 cites W147232447 @default.
• W3100802265 cites W1570622790 @default.
• W3100802265 cites W1966244186 @default.
• W3100802265 cites W1966373674 @default.
• W3100802265 cites W1973538702 @default.
• W3100802265 cites W1981030602 @default.
• W3100802265 cites W1987319691 @default.
• W3100802265 cites W1991610844 @default.
• W3100802265 cites W1991693518 @default.
• W3100802265 cites W1993357312 @default.
• W3100802265 cites W1998553272 @default.
• W3100802265 cites W2000566616 @default.
• W3100802265 cites W2011759989 @default.
• W3100802265 cites W2013305727 @default.
• W3100802265 cites W2017466075 @default.
• W3100802265 cites W2023344645 @default.
• W3100802265 cites W2026516601 @default.
• W3100802265 cites W2030244372 @default.
• W3100802265 cites W2031330193 @default.
• W3100802265 cites W2042767877 @default.
• W3100802265 cites W2043766240 @default.
• W3100802265 cites W2046831851 @default.
• W3100802265 cites W2050152520 @default.
• W3100802265 cites W2054753415 @default.
• W3100802265 cites W2060509649 @default.
• W3100802265 cites W2064576366 @default.
• W3100802265 cites W2082619949 @default.
• W3100802265 cites W2089583673 @default.
• W3100802265 cites W2096773796 @default.
• W3100802265 cites W2102030688 @default.
• W3100802265 cites W2102748293 @default.
• W3100802265 cites W2114945401 @default.
• W3100802265 cites W2128738047 @default.
• W3100802265 cites W2138534553 @default.
• W3100802265 cites W2145808393 @default.
• W3100802265 cites W2154397258 @default.
• W3100802265 cites W2166101527 @default.
• W3100802265 cites W2166931875 @default.
• W3100802265 cites W2169393734 @default.
• W3100802265 cites W2221977688 @default.
• W3100802265 cites W2286456170 @default.
• W3100802265 cites W2798336535 @default.
• W3100802265 cites W2802440906 @default.
• W3100802265 cites W2842352012 @default.
• W3100802265 cites W2883290686 @default.
• W3100802265 cites W2916355868 @default.
• W3100802265 cites W2933767048 @default.
• W3100802265 cites W3099520586 @default.
• W3100802265 cites W3099571084 @default.
• W3100802265 cites W3100369123 @default.
• W3100802265 cites W3100964914 @default.
• W3100802265 cites W3101534675 @default.
• W3100802265 cites W3102302291 @default.
• W3100802265 cites W3102419632 @default.
• W3100802265 cites W3103808404 @default.
• W3100802265 cites W3104435745 @default.
• W3100802265 cites W3104728055 @default.
• W3100802265 cites W3105593358 @default.
• W3100802265 cites W3122474463 @default.
• W3100802265 cites W3125137869 @default.
• W3100802265 cites W3125528990 @default.
• W3100802265 cites W4290961010 @default.
• W3100802265 cites W4292897694 @default.
• W3100802265 cites W4293241248 @default.
• W3100802265 doi "https://doi.org/10.3847/1538-4357/ab3a3f" @default.
• W3100802265 hasPublicationYear "2019" @default.
• W3100802265 type Work @default.
• W3100802265 sameAs 3100802265 @default.
• W3100802265 citedByCount "7" @default.
• W3100802265 countsByYear W31008022652022 @default.
• W3100802265 countsByYear W31008022652023 @default.
• W3100802265 crossrefType "journal-article" @default.
• W3100802265 hasAuthorship W3100802265A5013321503 @default.
• W3100802265 hasAuthorship W3100802265A5021958638 @default.
• W3100802265 hasBestOaLocation W31008022651 @default.
• W3100802265 hasConcept C121332964 @default.
• W3100802265 hasConcept C12287442 @default.
• W3100802265 hasConcept C125857072 @default.
• W3100802265 hasConcept C1276947 @default.
• W3100802265 hasConcept C150846664 @default.
• W3100802265 hasConcept C178075534 @default.
• W3100802265 hasConcept C23254167 @default.
• W3100802265 hasConcept C2776026020 @default.
• W3100802265 hasConcept C2776401274 @default.
• W3100802265 hasConcept C2779496878 @default.
• W3100802265 hasConcept C44870925 @default.
• W3100802265 hasConcept C98444146 @default.
• W3100802265 hasConceptScore W3100802265C121332964 @default.
• W3100802265 hasConceptScore W3100802265C12287442 @default.
• W3100802265 hasConceptScore W3100802265C125857072 @default.
• W3100802265 hasConceptScore W3100802265C1276947 @default.

• next