FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2023163408> ?p ?o ?g. }

• W2023163408 endingPage "133" @default.
• W2023163408 startingPage "123" @default.
• W2023163408 abstract "I modeled the 14 Å–37 μm SED of the recurrent symbiotic nova RS Oph during its supersoft source (SSS) phase and the following quiescent phase. During the SSS phase, the model SEDs revealed the presence of a strong stellar and nebular component of radiation in the spectrum. The former was emitted by the burning WD at highly super-Eddington rate, while the latter represented a fraction of its radiation reprocessed by the thermal nebula. During the transition phase, both the components were decreasing and during quiescence the SED satisfied radiation produced by a large, optically thick disk (Rdisk>10 R⊙). The super-Eddington luminosity of the burning WD during the SSS phase was independently justified by the high quantity of the nebular emission. The emitting material surrounded the burning WD, and its mass was (1.6±0.5)×10-4(d/1.6kpc)5/2 M⊙. The helium ash, deposited on the WD surface during the whole burning period, was around of 8×10-6(d/1.6kpc)2 M⊙, which yields an average growing rate of the WD mass, ṀWD∼4×10-7(d/1.6kpc)2 M⊙yr-1. The mass accreted by the WD between outbursts, macc∼1.26×10-5 M⊙, constrains the average accretion rate, Ṁacc∼6.3×10-7 M⊙yr-1. During quiescence, the accretion rate from the model SED of ∼2.3×10-7 M⊙yr-1 requires a super-Eddington accretion from the disk at ∼3.6×10-5 M⊙yr-1 during the outburst. Such a high accretion can be responsible for the super-Eddington luminosity during the whole burning phase. Simultaneous presence of jets supports this scenario. If the wind from the giant is not sufficient to feed the WD at the required rate, the accretion can be realized from the disk-like reservoir of material around the WD. In this case the time between outbursts will extend, with the next explosion beyond 2027. In the opposite case, the wind from the giant has to be focused to the orbital plane to sustain the high accretion rate at a few ×10-7 M⊙yr-1. Then the next explosion can occur even prior to 2027." @default.
• W2023163408 created "2016-06-24" @default.
• W2023163408 creator A5029409855 @default.
• W2023163408 date "2015-01-01" @default.
• W2023163408 modified "2023-09-30" @default.
• W2023163408 title "Multiwavelength modeling the SED of supersoft X-ray sources III. RS Ophiuchi: The supersoft X-ray phase and beyond" @default.
• W2023163408 cites W1963570574 @default.
• W2023163408 cites W1964596234 @default.
• W2023163408 cites W1970465431 @default.
• W2023163408 cites W1971749020 @default.
• W2023163408 cites W1972900570 @default.
• W2023163408 cites W1977356395 @default.
• W2023163408 cites W1977607328 @default.
• W2023163408 cites W1984800421 @default.
• W2023163408 cites W1991965092 @default.
• W2023163408 cites W1992015258 @default.
• W2023163408 cites W1997141843 @default.
• W2023163408 cites W1997248462 @default.
• W2023163408 cites W1998612705 @default.
• W2023163408 cites W1999315125 @default.
• W2023163408 cites W2015172002 @default.
• W2023163408 cites W2015506940 @default.
• W2023163408 cites W2027481605 @default.
• W2023163408 cites W2034657416 @default.
• W2023163408 cites W2036889949 @default.
• W2023163408 cites W2037104120 @default.
• W2023163408 cites W2051679034 @default.
• W2023163408 cites W2053715418 @default.
• W2023163408 cites W2057250782 @default.
• W2023163408 cites W2072637634 @default.
• W2023163408 cites W2079311823 @default.
• W2023163408 cites W2079756359 @default.
• W2023163408 cites W2086852367 @default.
• W2023163408 cites W2092949919 @default.
• W2023163408 cites W2100467488 @default.
• W2023163408 cites W2128136992 @default.
• W2023163408 cites W2130073501 @default.
• W2023163408 cites W2134788621 @default.
• W2023163408 cites W3099141784 @default.
• W2023163408 cites W3099302104 @default.
• W2023163408 cites W3099689618 @default.
• W2023163408 cites W3101097531 @default.
• W2023163408 cites W3103269013 @default.
• W2023163408 cites W3103286840 @default.
• W2023163408 cites W3103771291 @default.
• W2023163408 cites W3123112321 @default.
• W2023163408 cites W3207726085 @default.
• W2023163408 cites W4297063625 @default.
• W2023163408 doi "https://doi.org/10.1016/j.newast.2014.05.008" @default.
• W2023163408 hasPublicationYear "2015" @default.
• W2023163408 type Work @default.
• W2023163408 sameAs 2023163408 @default.
• W2023163408 citedByCount "5" @default.
• W2023163408 countsByYear W20231634082014 @default.
• W2023163408 countsByYear W20231634082015 @default.
• W2023163408 countsByYear W20231634082019 @default.
• W2023163408 countsByYear W20231634082022 @default.
• W2023163408 crossrefType "journal-article" @default.
• W2023163408 hasAuthorship W2023163408A5029409855 @default.
• W2023163408 hasBestOaLocation W20231634082 @default.
• W2023163408 hasConcept C117808444 @default.
• W2023163408 hasConcept C121332964 @default.
• W2023163408 hasConcept C12287442 @default.
• W2023163408 hasConcept C1276947 @default.
• W2023163408 hasConcept C2776401274 @default.
• W2023163408 hasConcept C44870925 @default.
• W2023163408 hasConcept C98444146 @default.
• W2023163408 hasConceptScore W2023163408C117808444 @default.
• W2023163408 hasConceptScore W2023163408C121332964 @default.
• W2023163408 hasConceptScore W2023163408C12287442 @default.
• W2023163408 hasConceptScore W2023163408C1276947 @default.
• W2023163408 hasConceptScore W2023163408C2776401274 @default.
• W2023163408 hasConceptScore W2023163408C44870925 @default.
• W2023163408 hasConceptScore W2023163408C98444146 @default.
• W2023163408 hasLocation W20231634081 @default.
• W2023163408 hasLocation W20231634082 @default.
• W2023163408 hasLocation W20231634083 @default.
• W2023163408 hasOpenAccess W2023163408 @default.
• W2023163408 hasPrimaryLocation W20231634081 @default.
• W2023163408 hasRelatedWork W1864702457 @default.
• W2023163408 hasRelatedWork W2047505318 @default.
• W2023163408 hasRelatedWork W2084146197 @default.
• W2023163408 hasRelatedWork W2464574710 @default.
• W2023163408 hasRelatedWork W2964944201 @default.
• W2023163408 hasRelatedWork W3103008063 @default.
• W2023163408 hasRelatedWork W3103046839 @default.
• W2023163408 hasRelatedWork W3125384449 @default.
• W2023163408 hasRelatedWork W3204427859 @default.
• W2023163408 hasRelatedWork W4286669523 @default.
• W2023163408 hasVolume "34" @default.
• W2023163408 isParatext "false" @default.
• W2023163408 isRetracted "false" @default.
• W2023163408 magId "2023163408" @default.
• W2023163408 workType "article" @default.