FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3100312017> ?p ?o ?g. }

• W3100312017 endingPage "A84" @default.
• W3100312017 startingPage "A84" @default.
• W3100312017 abstract "Since asymptotic giant branch (AGB) stars are bright and extended infrared objects, most Galactic AGB stars saturate the Wide-field Infrared Survey Explorer (WISE) detectors and therefore the WISE magnitudes that are restored by applying point-spread-function fitting need to be verified. Statistical properties of circumstellar envelopes around AGB stars are discussed on the basis of a WISE AGB catalog verified in this way. We cross-matched an AGB star sample with the WISE All-Sky Source Catalog and the Two Mircon All Sky Survey catalog. Infrared Space Observatory (ISO) spectra of a subsample of WISE AGB stars were also exploited. The dust radiation transfer code DUSTY was used to help predict the magnitudes in the W1 and W2 bands, the two WISE bands most affected by saturation, for calibration purpose, and to provide physical parameters of the AGB sample stars for analysis. DUSTY is verified against the ISO spectra to be a good tool to reproduce the spectral energy distributions of these AGB stars. Systematic magnitude-dependent offsets have been identified in WISE W1 and W2 magnitudes of the saturated AGB stars, and empirical calibration formulas are obtained for them on the basis of 1877 (W1) and 1558 (W2) AGB stars that are successfully fit with DUSTY. According to the calibration formulae, the corrections for W1 at 5 mag and W2 at 4 mag are $-0.383$ and 0.217 mag, respectively. In total, we calibrated the W1/W2 magnitudes of 2390/2021 AGB stars. The model parameters from the DUSTY and the calibrated WISE W1 and W2 magnitudes are used to discuss the behavior of the WISE color-color diagrams of AGB stars. The model parameters also reveal that O-rich AGB stars with opaque circumstellar envelopes are much rarer than opaque C-rich AGB stars toward the anti-Galactic center direction, which we attribute to the metallicity gradient of our Galaxy." @default.
• W3100312017 created "2020-11-23" @default.
• W3100312017 creator A5035399113 @default.
• W3100312017 creator A5046920270 @default.
• W3100312017 creator A5073008031 @default.
• W3100312017 creator A5074802467 @default.
• W3100312017 date "2014-04-01" @default.
• W3100312017 modified "2023-10-16" @default.
• W3100312017 title "Characterizing AGB stars in Wide-field Infrared Survey Explorer (WISE) bands" @default.
• W3100312017 cites W1626149790 @default.
• W3100312017 cites W1965372241 @default.
• W3100312017 cites W1982110912 @default.
• W3100312017 cites W1984455337 @default.
• W3100312017 cites W1985317931 @default.
• W3100312017 cites W2000310956 @default.
• W3100312017 cites W2006487645 @default.
• W3100312017 cites W2025358604 @default.
• W3100312017 cites W2027951065 @default.
• W3100312017 cites W2049774312 @default.
• W3100312017 cites W2052937506 @default.
• W3100312017 cites W2058633551 @default.
• W3100312017 cites W2067014603 @default.
• W3100312017 cites W2070362623 @default.
• W3100312017 cites W2071965568 @default.
• W3100312017 cites W2074940377 @default.
• W3100312017 cites W2086233841 @default.
• W3100312017 cites W2095224134 @default.
• W3100312017 cites W2103973422 @default.
• W3100312017 cites W2104584484 @default.
• W3100312017 cites W2109793665 @default.
• W3100312017 cites W2124565542 @default.
• W3100312017 cites W2128533239 @default.
• W3100312017 cites W2142220522 @default.
• W3100312017 cites W2143213816 @default.
• W3100312017 cites W2150283860 @default.
• W3100312017 cites W2164520001 @default.
• W3100312017 cites W3099270657 @default.
• W3100312017 cites W3101126610 @default.
• W3100312017 cites W3101768765 @default.
• W3100312017 cites W3102710086 @default.
• W3100312017 cites W3103989567 @default.
• W3100312017 cites W3105730088 @default.
• W3100312017 cites W3105751689 @default.
• W3100312017 cites W3125645638 @default.
• W3100312017 cites W4247735440 @default.
• W3100312017 cites W4251046729 @default.
• W3100312017 cites W4294255512 @default.
• W3100312017 cites W4298293878 @default.
• W3100312017 doi "https://doi.org/10.1051/0004-6361/201322818" @default.
• W3100312017 hasPublicationYear "2014" @default.
• W3100312017 type Work @default.
• W3100312017 sameAs 3100312017 @default.
• W3100312017 citedByCount "12" @default.
• W3100312017 countsByYear W31003120172017 @default.
• W3100312017 countsByYear W31003120172018 @default.
• W3100312017 countsByYear W31003120172019 @default.
• W3100312017 countsByYear W31003120172020 @default.
• W3100312017 countsByYear W31003120172021 @default.
• W3100312017 countsByYear W31003120172022 @default.
• W3100312017 countsByYear W31003120172023 @default.
• W3100312017 crossrefType "journal-article" @default.
• W3100312017 hasAuthorship W3100312017A5035399113 @default.
• W3100312017 hasAuthorship W3100312017A5046920270 @default.
• W3100312017 hasAuthorship W3100312017A5073008031 @default.
• W3100312017 hasAuthorship W3100312017A5074802467 @default.
• W3100312017 hasBestOaLocation W31003120171 @default.
• W3100312017 hasConcept C121332964 @default.
• W3100312017 hasConcept C1276947 @default.
• W3100312017 hasConcept C150846664 @default.
• W3100312017 hasConcept C158355884 @default.
• W3100312017 hasConcept C181313176 @default.
• W3100312017 hasConcept C2779919027 @default.
• W3100312017 hasConcept C44870925 @default.
• W3100312017 hasConcept C73329638 @default.
• W3100312017 hasConceptScore W3100312017C121332964 @default.
• W3100312017 hasConceptScore W3100312017C1276947 @default.
• W3100312017 hasConceptScore W3100312017C150846664 @default.
• W3100312017 hasConceptScore W3100312017C158355884 @default.
• W3100312017 hasConceptScore W3100312017C181313176 @default.
• W3100312017 hasConceptScore W3100312017C2779919027 @default.
• W3100312017 hasConceptScore W3100312017C44870925 @default.
• W3100312017 hasConceptScore W3100312017C73329638 @default.
• W3100312017 hasLocation W31003120171 @default.
• W3100312017 hasLocation W31003120172 @default.
• W3100312017 hasLocation W31003120173 @default.
• W3100312017 hasLocation W31003120174 @default.
• W3100312017 hasLocation W31003120175 @default.
• W3100312017 hasOpenAccess W3100312017 @default.
• W3100312017 hasPrimaryLocation W31003120171 @default.
• W3100312017 hasRelatedWork W1978739134 @default.
• W3100312017 hasRelatedWork W1986109513 @default.
• W3100312017 hasRelatedWork W1994702306 @default.
• W3100312017 hasRelatedWork W2006993921 @default.
• W3100312017 hasRelatedWork W2028715815 @default.
• W3100312017 hasRelatedWork W2031284670 @default.
• W3100312017 hasRelatedWork W2164171155 @default.
• W3100312017 hasRelatedWork W2259654192 @default.
• W3100312017 hasRelatedWork W3099976984 @default.

• next