FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2111569458> ?p ?o ?g. }

• W2111569458 endingPage "L40" @default.
• W2111569458 startingPage "L37" @default.
• W2111569458 abstract "We have analyzed an XMM-Newton observation of the nearby spiral galaxy NGC 1313, which contains two ultraluminous X-ray (ULX) sources. We measure isotropic luminosities of LX = 2.0 × 1040 ergs s-1 and LX = 6.6 × 1039 ergs s-1 for NGC 1313 X-1 and X-2 (0.2-10.0 keV, assuming a distance of 3.7 Mpc). The spectra statistically require soft and hard spectral components to describe the continuum emission; some prior studies of ULX sources have claimed cool soft components with lower statistics. The improvement over several single-component models exceeds the 8 σ level of confidence for X-1; the improvement for X-2 is significant at the 3 σ level. The soft components in these ULX spectra are well fitted by multicolor disk blackbody models with color temperatures of kT ≃ 150 eV. This temperature differs markedly from those commonly measured in the spectra of stellar mass (10 M☉) black holes in their brightest states (kT ≃ 1 keV). It is expected that the temperature of an accretion disk orbiting a black hole should decrease with increasing black hole mass. If the soft components we measure are due to emission from the inner region of an accretion disk, and disks extend close to the innermost stable circular orbit at the accretion rates being probed, the low color temperatures may be interpreted as spectroscopic evidence of black holes with intermediate masses: MBH ≃ 103 M☉. Simple Eddington scaling arguments suggest a minimum mass of MBH ~ 102 M☉. NGC 1313 X-1 and X-2 are found in optical nebulae, which may indicate that anisotropic emission geometries are unlikely to account for the fluxes observed." @default.
• W2111569458 created "2016-06-24" @default.
• W2111569458 creator A5024983697 @default.
• W2111569458 creator A5025039442 @default.
• W2111569458 creator A5028370726 @default.
• W2111569458 creator A5080029324 @default.
• W2111569458 date "2003-03-01" @default.
• W2111569458 modified "2023-10-15" @default.
• W2111569458 title "X-Ray Spectroscopic Evidence for Intermediate-Mass Black Holes: Cool Accretion Disks in Two Ultraluminous X-Ray Sources" @default.
• W2111569458 cites W2008281661 @default.
• W2111569458 cites W2022598858 @default.
• W2111569458 cites W2035225065 @default.
• W2111569458 cites W2040573793 @default.
• W2111569458 cites W2075239744 @default.
• W2111569458 cites W2084087407 @default.
• W2111569458 cites W2088819227 @default.
• W2111569458 cites W2123602663 @default.
• W2111569458 cites W2124131920 @default.
• W2111569458 cites W2144890838 @default.
• W2111569458 cites W2149710854 @default.
• W2111569458 cites W2161056181 @default.
• W2111569458 cites W2164570275 @default.
• W2111569458 cites W2985443361 @default.
• W2111569458 cites W3097987127 @default.
• W2111569458 cites W3099094606 @default.
• W2111569458 cites W3104379663 @default.
• W2111569458 cites W3106024153 @default.
• W2111569458 cites W3125275757 @default.
• W2111569458 cites W4290707612 @default.
• W2111569458 doi "https://doi.org/10.1086/368373" @default.
• W2111569458 hasPublicationYear "2003" @default.
• W2111569458 type Work @default.
• W2111569458 sameAs 2111569458 @default.
• W2111569458 citedByCount "246" @default.
• W2111569458 countsByYear W21115694582012 @default.
• W2111569458 countsByYear W21115694582013 @default.
• W2111569458 countsByYear W21115694582014 @default.
• W2111569458 countsByYear W21115694582015 @default.
• W2111569458 countsByYear W21115694582016 @default.
• W2111569458 countsByYear W21115694582017 @default.
• W2111569458 countsByYear W21115694582018 @default.
• W2111569458 countsByYear W21115694582019 @default.
• W2111569458 countsByYear W21115694582020 @default.
• W2111569458 countsByYear W21115694582021 @default.
• W2111569458 countsByYear W21115694582022 @default.
• W2111569458 countsByYear W21115694582023 @default.
• W2111569458 crossrefType "journal-article" @default.
• W2111569458 hasAuthorship W2111569458A5024983697 @default.
• W2111569458 hasAuthorship W2111569458A5025039442 @default.
• W2111569458 hasAuthorship W2111569458A5028370726 @default.
• W2111569458 hasAuthorship W2111569458A5080029324 @default.
• W2111569458 hasBestOaLocation W21115694581 @default.
• W2111569458 hasConcept C104954878 @default.
• W2111569458 hasConcept C121332964 @default.
• W2111569458 hasConcept C1276947 @default.
• W2111569458 hasConcept C153385146 @default.
• W2111569458 hasConcept C157909335 @default.
• W2111569458 hasConcept C2776401274 @default.
• W2111569458 hasConcept C31258907 @default.
• W2111569458 hasConcept C41008148 @default.
• W2111569458 hasConcept C44870925 @default.
• W2111569458 hasConcept C4839761 @default.
• W2111569458 hasConcept C50341732 @default.
• W2111569458 hasConcept C62520636 @default.
• W2111569458 hasConcept C74172769 @default.
• W2111569458 hasConcept C89305328 @default.
• W2111569458 hasConcept C98444146 @default.
• W2111569458 hasConceptScore W2111569458C104954878 @default.
• W2111569458 hasConceptScore W2111569458C121332964 @default.
• W2111569458 hasConceptScore W2111569458C1276947 @default.
• W2111569458 hasConceptScore W2111569458C153385146 @default.
• W2111569458 hasConceptScore W2111569458C157909335 @default.
• W2111569458 hasConceptScore W2111569458C2776401274 @default.
• W2111569458 hasConceptScore W2111569458C31258907 @default.
• W2111569458 hasConceptScore W2111569458C41008148 @default.
• W2111569458 hasConceptScore W2111569458C44870925 @default.
• W2111569458 hasConceptScore W2111569458C4839761 @default.
• W2111569458 hasConceptScore W2111569458C50341732 @default.
• W2111569458 hasConceptScore W2111569458C62520636 @default.
• W2111569458 hasConceptScore W2111569458C74172769 @default.
• W2111569458 hasConceptScore W2111569458C89305328 @default.
• W2111569458 hasConceptScore W2111569458C98444146 @default.
• W2111569458 hasIssue "1" @default.
• W2111569458 hasLocation W21115694581 @default.
• W2111569458 hasOpenAccess W2111569458 @default.
• W2111569458 hasPrimaryLocation W21115694581 @default.
• W2111569458 hasRelatedWork W119351016 @default.
• W2111569458 hasRelatedWork W2073227327 @default.
• W2111569458 hasRelatedWork W2079391868 @default.
• W2111569458 hasRelatedWork W2117359402 @default.
• W2111569458 hasRelatedWork W2351712597 @default.
• W2111569458 hasRelatedWork W2358134341 @default.
• W2111569458 hasRelatedWork W2381644775 @default.
• W2111569458 hasRelatedWork W2552592440 @default.
• W2111569458 hasRelatedWork W2616284033 @default.
• W2111569458 hasRelatedWork W4286005541 @default.
• W2111569458 hasVolume "585" @default.
• W2111569458 isParatext "false" @default.

• next