FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W1997372286> ?p ?o ?g. }

• W1997372286 endingPage "1479" @default.
• W1997372286 startingPage "1473" @default.
• W1997372286 abstract "With XMM-Newton and the Spitzer Space Telescope, we obtain upper bounds to the X-ray fluxes from G29-38 and GD 362, and the 70 μm flux from G29-38. These data provide indirect evidence that G29-38 is accreting from a tidally disrupted asteroid: it is neither accreting large amounts of hydrogen and helium nor is its surrounding dusty disk being replenished from a reservoir of cold grains experiencing Poynting–Robertson drag. The upper bound to the X-ray flux from GD 362 is consistent with the estimated rate of mass accretion required to explain its pollution by elements heavier than helium. GD 362 also possesses 0.01 M⊕ of hydrogen, an anomalously large amount for a white dwarf with a helium-dominated atmosphere. One possibility is that before the current disk was formed, this hydrogen was accreted either from ∼100 Ceres-like asteroids or one large object. An alternative scenario which simultaneously explains all of GD 362's distinctive properties is that we are witnessing the consequences of the tidal destruction of a single parent body that had internal water and was at least as massive as Callisto and probably as massive as Mars." @default.
• W1997372286 created "2016-06-24" @default.
• W1997372286 creator A5023556781 @default.
• W1997372286 creator A5065761076 @default.
• W1997372286 creator A5065769453 @default.
• W1997372286 creator A5075607587 @default.
• W1997372286 date "2009-06-23" @default.
• W1997372286 modified "2023-09-27" @default.
• W1997372286 title "X-RAY AND INFRARED OBSERVATIONS OF TWO EXTERNALLY POLLUTED WHITE DWARFS" @default.
• W1997372286 cites W1485073943 @default.
• W1997372286 cites W1757987097 @default.
• W1997372286 cites W1988559221 @default.
• W1997372286 cites W1992561743 @default.
• W1997372286 cites W1996228609 @default.
• W1997372286 cites W1996564807 @default.
• W1997372286 cites W2008957594 @default.
• W1997372286 cites W2017761991 @default.
• W1997372286 cites W2018982227 @default.
• W1997372286 cites W2028678583 @default.
• W1997372286 cites W2030227402 @default.
• W1997372286 cites W2037544596 @default.
• W1997372286 cites W2043365644 @default.
• W1997372286 cites W2044669640 @default.
• W1997372286 cites W2048233625 @default.
• W1997372286 cites W2048506031 @default.
• W1997372286 cites W2049324094 @default.
• W1997372286 cites W2050990551 @default.
• W1997372286 cites W2055124830 @default.
• W1997372286 cites W2055834769 @default.
• W1997372286 cites W2063819537 @default.
• W1997372286 cites W2066891664 @default.
• W1997372286 cites W2067984861 @default.
• W1997372286 cites W2077134158 @default.
• W1997372286 cites W2078883760 @default.
• W1997372286 cites W2084110536 @default.
• W1997372286 cites W2086347583 @default.
• W1997372286 cites W2086841799 @default.
• W1997372286 cites W2093189371 @default.
• W1997372286 cites W2093397420 @default.
• W1997372286 cites W2100259324 @default.
• W1997372286 cites W2102145402 @default.
• W1997372286 cites W2109870426 @default.
• W1997372286 cites W2120176236 @default.
• W1997372286 cites W2122237670 @default.
• W1997372286 cites W2131666994 @default.
• W1997372286 cites W2132142743 @default.
• W1997372286 cites W2140944900 @default.
• W1997372286 cites W2154078330 @default.
• W1997372286 cites W2167345633 @default.
• W1997372286 cites W3086206496 @default.
• W1997372286 cites W3099270657 @default.
• W1997372286 cites W3099490864 @default.
• W1997372286 cites W3100224081 @default.
• W1997372286 cites W3101520660 @default.
• W1997372286 cites W3101564605 @default.
• W1997372286 cites W3101807314 @default.
• W1997372286 cites W3102118201 @default.
• W1997372286 cites W3102426331 @default.
• W1997372286 cites W3126085942 @default.
• W1997372286 cites W4293438942 @default.
• W1997372286 cites W48926618 @default.
• W1997372286 doi "https://doi.org/10.1088/0004-637x/699/2/1473" @default.
• W1997372286 hasPublicationYear "2009" @default.
• W1997372286 type Work @default.
• W1997372286 sameAs 1997372286 @default.
• W1997372286 citedByCount "69" @default.
• W1997372286 countsByYear W19973722862012 @default.
• W1997372286 countsByYear W19973722862013 @default.
• W1997372286 countsByYear W19973722862014 @default.
• W1997372286 countsByYear W19973722862015 @default.
• W1997372286 countsByYear W19973722862016 @default.
• W1997372286 countsByYear W19973722862017 @default.
• W1997372286 countsByYear W19973722862018 @default.
• W1997372286 countsByYear W19973722862019 @default.
• W1997372286 countsByYear W19973722862020 @default.
• W1997372286 countsByYear W19973722862021 @default.
• W1997372286 countsByYear W19973722862022 @default.
• W1997372286 countsByYear W19973722862023 @default.
• W1997372286 crossrefType "journal-article" @default.
• W1997372286 hasAuthorship W1997372286A5023556781 @default.
• W1997372286 hasAuthorship W1997372286A5065761076 @default.
• W1997372286 hasAuthorship W1997372286A5065769453 @default.
• W1997372286 hasAuthorship W1997372286A5075607587 @default.
• W1997372286 hasBestOaLocation W19973722861 @default.
• W1997372286 hasConcept C121332964 @default.
• W1997372286 hasConcept C1276947 @default.
• W1997372286 hasConcept C150846664 @default.
• W1997372286 hasConcept C184779094 @default.
• W1997372286 hasConcept C191897082 @default.
• W1997372286 hasConcept C192562407 @default.
• W1997372286 hasConcept C197445014 @default.
• W1997372286 hasConcept C2776401274 @default.
• W1997372286 hasConcept C44870925 @default.
• W1997372286 hasConcept C51244244 @default.
• W1997372286 hasConcept C522977591 @default.
• W1997372286 hasConcept C546029482 @default.
• W1997372286 hasConcept C58142911 @default.
• W1997372286 hasConcept C68709404 @default.

• next