FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W1972214728> ?p ?o ?g. }

• W1972214728 abstract "We focus here on one particular and poorly studied object, IRAS11472-0800. It is a highly evolved post-Asymptotic Giant Branch (post-AGB) star of spectral type F, with a large infrared excess produced by thermal emission of circumstellar dust. We deploy a multi-wavelength study which includes the analyses of optical and IR spectra as well as a variability study based on photometric and spectroscopic time-series. The spectral energy distribution (SED) properties as well as the highly processed silicate N-band emission show that the dust in IRAS11472-0800 is likely trapped in a stable disc. The energetics of the SED and the colour variability show that our viewing angle is close to edge-on and that the optical flux is dominated by scattered light. With photospheric abundances of [Fe/H] = -2.7 and [Sc/H]=-4.2, we discovered that IRAS11472-0800 is one of the most chemically-depleted objects known to date. Moreover, IRAS11472-0800 is a pulsating star with a period of 31.16 days and a peak-to-peak amplitude of 0.6 mag in V. The radial velocity variability is strongly influenced by the pulsations, but the significant cycle-to-cycle variability is systematic on a longer time scale, which we interpret as evidence for binary motion. We conclude that IRAS11472-0800 is a pulsating binary star surrounded by a circumbinary disc. The line-of-sight towards the object lies close the the orbital plane making that the optical light is dominated by scattered light. IRAS11472-0800 is one of the most chemically-depleted objects known so far and links the dusty RV,Tauri stars to the non-pulsating class of strongly depleted objects." @default.
• W1972214728 created "2016-06-24" @default.
• W1972214728 creator A5003343919 @default.
• W1972214728 creator A5028996824 @default.
• W1972214728 creator A5056099322 @default.
• W1972214728 creator A5066643989 @default.
• W1972214728 creator A5076564877 @default.
• W1972214728 date "2012-06-01" @default.
• W1972214728 modified "2023-10-14" @default.
• W1972214728 title "IRAS 11472−0800: an extremely depleted pulsating binary post-AGB star" @default.
• W1972214728 cites W1661200856 @default.
• W1972214728 cites W1739387363 @default.
• W1972214728 cites W1790922966 @default.
• W1972214728 cites W1970520663 @default.
• W1972214728 cites W1973932881 @default.
• W1972214728 cites W1974913150 @default.
• W1972214728 cites W1981833741 @default.
• W1972214728 cites W2000303492 @default.
• W1972214728 cites W2002700218 @default.
• W1972214728 cites W2008047110 @default.
• W1972214728 cites W2009217756 @default.
• W1972214728 cites W2013859371 @default.
• W1972214728 cites W201620497 @default.
• W1972214728 cites W2019813542 @default.
• W1972214728 cites W2025397185 @default.
• W1972214728 cites W2029985887 @default.
• W1972214728 cites W2031487684 @default.
• W1972214728 cites W2057641281 @default.
• W1972214728 cites W2072978424 @default.
• W1972214728 cites W2075292177 @default.
• W1972214728 cites W2083592425 @default.
• W1972214728 cites W2086209426 @default.
• W1972214728 cites W2088675366 @default.
• W1972214728 cites W2096471541 @default.
• W1972214728 cites W2099724889 @default.
• W1972214728 cites W2109519881 @default.
• W1972214728 cites W2112612199 @default.
• W1972214728 cites W2120123803 @default.
• W1972214728 cites W2121316478 @default.
• W1972214728 cites W2140449099 @default.
• W1972214728 cites W2141070818 @default.
• W1972214728 cites W2142220522 @default.
• W1972214728 cites W2149889006 @default.
• W1972214728 cites W2152129350 @default.
• W1972214728 cites W2160092266 @default.
• W1972214728 cites W2899497983 @default.
• W1972214728 cites W3098483518 @default.
• W1972214728 cites W3098603160 @default.
• W1972214728 cites W3099032735 @default.
• W1972214728 cites W3100016480 @default.
• W1972214728 cites W3101364261 @default.
• W1972214728 cites W3101671574 @default.
• W1972214728 cites W3104204533 @default.
• W1972214728 cites W3104882191 @default.
• W1972214728 cites W3106147843 @default.
• W1972214728 cites W94987512 @default.
• W1972214728 doi "https://doi.org/10.1051/0004-6361/201218835" @default.
• W1972214728 hasPublicationYear "2012" @default.
• W1972214728 type Work @default.
• W1972214728 sameAs 1972214728 @default.
• W1972214728 citedByCount "12" @default.
• W1972214728 countsByYear W19722147282013 @default.
• W1972214728 countsByYear W19722147282014 @default.
• W1972214728 countsByYear W19722147282015 @default.
• W1972214728 countsByYear W19722147282017 @default.
• W1972214728 countsByYear W19722147282019 @default.
• W1972214728 countsByYear W19722147282020 @default.
• W1972214728 countsByYear W19722147282021 @default.
• W1972214728 crossrefType "journal-article" @default.
• W1972214728 hasAuthorship W1972214728A5003343919 @default.
• W1972214728 hasAuthorship W1972214728A5028996824 @default.
• W1972214728 hasAuthorship W1972214728A5056099322 @default.
• W1972214728 hasAuthorship W1972214728A5066643989 @default.
• W1972214728 hasAuthorship W1972214728A5076564877 @default.
• W1972214728 hasBestOaLocation W19722147282 @default.
• W1972214728 hasConcept C10632323 @default.
• W1972214728 hasConcept C120665830 @default.
• W1972214728 hasConcept C121332964 @default.
• W1972214728 hasConcept C1276947 @default.
• W1972214728 hasConcept C14427944 @default.
• W1972214728 hasConcept C150846664 @default.
• W1972214728 hasConcept C180205008 @default.
• W1972214728 hasConcept C181313176 @default.
• W1972214728 hasConcept C191897082 @default.
• W1972214728 hasConcept C192562407 @default.
• W1972214728 hasConcept C198352243 @default.
• W1972214728 hasConcept C2524010 @default.
• W1972214728 hasConcept C2780928442 @default.
• W1972214728 hasConcept C33923547 @default.
• W1972214728 hasConcept C41074950 @default.
• W1972214728 hasConcept C44870925 @default.
• W1972214728 hasConcept C48372109 @default.
• W1972214728 hasConcept C4839761 @default.
• W1972214728 hasConcept C50425793 @default.
• W1972214728 hasConcept C6260449 @default.
• W1972214728 hasConcept C68709404 @default.
• W1972214728 hasConcept C8865038 @default.
• W1972214728 hasConcept C94375191 @default.
• W1972214728 hasConceptScore W1972214728C10632323 @default.
• W1972214728 hasConceptScore W1972214728C120665830 @default.

• next