Matches in SemOpenAlex for { <https://semopenalex.org/work/W2005372226> ?p ?o ?g. }
- W2005372226 abstract "Abstract X-ray observations have shown that, like all late-type stars, young, low-mass stars are magnetized. X-ray flaring characteristics suggest that the resulting activity is solar-like, with X-ray emission coming from a hot plasma confined in large, reconnecting magnetic loops. On the other hand, except at late stages of their pre-main sequence evolution, young stars are surrounded by circumstellar material, disks and outflows. This review describes current theoretical ideas in which the magnetic field, in particular in the star-disk region, converts accretion from the disks into outflow ejection, and how some theories allow us to predict X-rays from reconnection-induced plasma heating. However, the search for direct X-ray evidence of star-disk interactions, as a partial test of accretion-ejection models, remains so far inconclusive. Accretion disks may play a role in the coronal activity of young stars, but this activity seems to be largely dominated by their solar-like, convection driven, magnetic activity." @default.
- W2005372226 created "2016-06-24" @default.
- W2005372226 creator A5038847773 @default.
- W2005372226 date "2003-09-01" @default.
- W2005372226 modified "2023-09-23" @default.
- W2005372226 title "The role of accretion disks in the coronal activity of young stars" @default.
- W2005372226 cites W12311309 @default.
- W2005372226 cites W1502649899 @default.
- W2005372226 cites W1571939782 @default.
- W2005372226 cites W1614857764 @default.
- W2005372226 cites W1642880642 @default.
- W2005372226 cites W1650658307 @default.
- W2005372226 cites W1653750365 @default.
- W2005372226 cites W1953859610 @default.
- W2005372226 cites W1964052401 @default.
- W2005372226 cites W1966244186 @default.
- W2005372226 cites W1968777507 @default.
- W2005372226 cites W1971535933 @default.
- W2005372226 cites W1978391636 @default.
- W2005372226 cites W1979218713 @default.
- W2005372226 cites W1988828220 @default.
- W2005372226 cites W1991214217 @default.
- W2005372226 cites W1999807917 @default.
- W2005372226 cites W2000417483 @default.
- W2005372226 cites W2006540157 @default.
- W2005372226 cites W2012482246 @default.
- W2005372226 cites W2013305727 @default.
- W2005372226 cites W2014437139 @default.
- W2005372226 cites W2026516601 @default.
- W2005372226 cites W2028194126 @default.
- W2005372226 cites W2032132855 @default.
- W2005372226 cites W2037536810 @default.
- W2005372226 cites W2041445436 @default.
- W2005372226 cites W2042151988 @default.
- W2005372226 cites W2042336801 @default.
- W2005372226 cites W2042753720 @default.
- W2005372226 cites W2044451815 @default.
- W2005372226 cites W2046452618 @default.
- W2005372226 cites W2048206028 @default.
- W2005372226 cites W2049325212 @default.
- W2005372226 cites W2055531005 @default.
- W2005372226 cites W2055793042 @default.
- W2005372226 cites W2055896295 @default.
- W2005372226 cites W2060025968 @default.
- W2005372226 cites W2062522010 @default.
- W2005372226 cites W2071186571 @default.
- W2005372226 cites W2081240748 @default.
- W2005372226 cites W2082546665 @default.
- W2005372226 cites W2087993597 @default.
- W2005372226 cites W2093494526 @default.
- W2005372226 cites W2127825363 @default.
- W2005372226 cites W2135280725 @default.
- W2005372226 cites W2138715692 @default.
- W2005372226 cites W2143714973 @default.
- W2005372226 cites W2164412465 @default.
- W2005372226 cites W2166931875 @default.
- W2005372226 cites W2171088869 @default.
- W2005372226 cites W2986674497 @default.
- W2005372226 cites W2989854654 @default.
- W2005372226 cites W2999560553 @default.
- W2005372226 cites W3095674797 @default.
- W2005372226 cites W3098712785 @default.
- W2005372226 cites W3098975237 @default.
- W2005372226 cites W3100140230 @default.
- W2005372226 cites W3100899479 @default.
- W2005372226 cites W3101376423 @default.
- W2005372226 cites W3102171918 @default.
- W2005372226 cites W3103994482 @default.
- W2005372226 cites W3104242243 @default.
- W2005372226 cites W3104702592 @default.
- W2005372226 cites W3106192446 @default.
- W2005372226 cites W3125845515 @default.
- W2005372226 cites W3137153919 @default.
- W2005372226 cites W343244306 @default.
- W2005372226 doi "https://doi.org/10.1016/s0273-1177(03)80067-4" @default.
- W2005372226 hasPublicationYear "2003" @default.
- W2005372226 type Work @default.
- W2005372226 sameAs 2005372226 @default.
- W2005372226 citedByCount "4" @default.
- W2005372226 countsByYear W20053722262019 @default.
- W2005372226 crossrefType "journal-article" @default.
- W2005372226 hasAuthorship W2005372226A5038847773 @default.
- W2005372226 hasConcept C115260700 @default.
- W2005372226 hasConcept C121332964 @default.
- W2005372226 hasConcept C1276947 @default.
- W2005372226 hasConcept C150846664 @default.
- W2005372226 hasConcept C153294291 @default.
- W2005372226 hasConcept C178075534 @default.
- W2005372226 hasConcept C195803813 @default.
- W2005372226 hasConcept C2776401274 @default.
- W2005372226 hasConcept C44870925 @default.
- W2005372226 hasConcept C56956389 @default.
- W2005372226 hasConcept C62520636 @default.
- W2005372226 hasConcept C82706917 @default.
- W2005372226 hasConcept C86132830 @default.
- W2005372226 hasConceptScore W2005372226C115260700 @default.
- W2005372226 hasConceptScore W2005372226C121332964 @default.
- W2005372226 hasConceptScore W2005372226C1276947 @default.
- W2005372226 hasConceptScore W2005372226C150846664 @default.
- W2005372226 hasConceptScore W2005372226C153294291 @default.