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• W2008132488 startingPage "462" @default.
• W2008132488 abstract "We present a new model-independent method of comparison of NIR visibility data of YSOs. The method is based on scaling the measured baseline with the YSO's distance and luminosity, which removes the dependence of visibility on these two variables. We use this method to compare all available NIR visibility data and demonstrate that it distinguishes YSOs of luminosity L⋆ ≲ 103 L☉ (low L) from YSOs of L⋆ ≳ 103 L☉ (high L). This confirms earlier suggestions, based on fits of image models to the visibility data, for the difference between the NIR sizes of these two luminosity groups. When plotted against the scaled baseline, the visibility creates the following data clusters: low-L Herbig Ae/Be stars, T Tauri stars, and high-L Herbig Be stars. We model the shape and size of clusters with different image models and find that low-L Herbig stars are best explained by the uniform brightness ring and the halo model, T Tauri stars with the halo model, and high-L Herbig stars with the accretion disk model. However, the plausibility of each model is not well established. Therefore, we try to build a descriptive model of the circumstellar environment consistent with various observed properties of YSOs. We argue that low-L YSOs have optically thick disks with the optically thin inner dust sublimation cavity and an optically thin dusty outflow above the inner disk regions. High-L YSOs have optically thick accretion disks with high accretion rates enabling gas to dominate the NIR emission over dust. Although observations would favor such a description of YSOs, the required dust distribution is not supported by our current understanding of dust dynamics." @default.
• W2008132488 created "2016-06-24" @default.
• W2008132488 creator A5005357545 @default.
• W2008132488 creator A5010933156 @default.
• W2008132488 date "2007-03-20" @default.
• W2008132488 modified "2023-09-29" @default.
• W2008132488 title "Relation between the Luminosity of Young Stellar Objects and Their Circumstellar Environment" @default.
• W2008132488 cites W1549448735 @default.
• W2008132488 cites W1657791533 @default.
• W2008132488 cites W1739387363 @default.
• W2008132488 cites W1964945577 @default.
• W2008132488 cites W1969860951 @default.
• W2008132488 cites W1971049572 @default.
• W2008132488 cites W1972763990 @default.
• W2008132488 cites W1975298624 @default.
• W2008132488 cites W1976807478 @default.
• W2008132488 cites W1978050287 @default.
• W2008132488 cites W1980610146 @default.
• W2008132488 cites W1981061070 @default.
• W2008132488 cites W1981800857 @default.
• W2008132488 cites W1983509013 @default.
• W2008132488 cites W1987938308 @default.
• W2008132488 cites W1989032480 @default.
• W2008132488 cites W1994985948 @default.
• W2008132488 cites W1998673955 @default.
• W2008132488 cites W2000548943 @default.
• W2008132488 cites W2004955121 @default.
• W2008132488 cites W2005467021 @default.
• W2008132488 cites W2010720514 @default.
• W2008132488 cites W2011292167 @default.
• W2008132488 cites W2016164487 @default.
• W2008132488 cites W2016301569 @default.
• W2008132488 cites W2024129150 @default.
• W2008132488 cites W2027135516 @default.
• W2008132488 cites W2027710352 @default.
• W2008132488 cites W2028855598 @default.
• W2008132488 cites W2029780970 @default.
• W2008132488 cites W2037345895 @default.
• W2008132488 cites W2038472758 @default.
• W2008132488 cites W2038760862 @default.
• W2008132488 cites W2043103621 @default.
• W2008132488 cites W2043689435 @default.
• W2008132488 cites W2044419757 @default.
• W2008132488 cites W2047379513 @default.
• W2008132488 cites W2047647423 @default.
• W2008132488 cites W2047754542 @default.
• W2008132488 cites W2047971340 @default.
• W2008132488 cites W2052248972 @default.
• W2008132488 cites W2053648858 @default.
• W2008132488 cites W2055112665 @default.
• W2008132488 cites W2059139406 @default.
• W2008132488 cites W2062303902 @default.
• W2008132488 cites W2063492181 @default.
• W2008132488 cites W2067886765 @default.
• W2008132488 cites W2075237489 @default.
• W2008132488 cites W2080430275 @default.
• W2008132488 cites W2080708236 @default.
• W2008132488 cites W2081303399 @default.
• W2008132488 cites W2083865471 @default.
• W2008132488 cites W2086180078 @default.
• W2008132488 cites W2091353304 @default.
• W2008132488 cites W2094956375 @default.
• W2008132488 cites W2095088858 @default.
• W2008132488 cites W2102352101 @default.
• W2008132488 cites W2103861147 @default.
• W2008132488 cites W2107028611 @default.
• W2008132488 cites W2110894057 @default.
• W2008132488 cites W2112156567 @default.
• W2008132488 cites W2113678655 @default.
• W2008132488 cites W2114945401 @default.
• W2008132488 cites W2116952160 @default.
• W2008132488 cites W2118958278 @default.
• W2008132488 cites W2127867276 @default.
• W2008132488 cites W2132400017 @default.
• W2008132488 cites W2132564213 @default.
• W2008132488 cites W2133389631 @default.
• W2008132488 cites W2150465135 @default.
• W2008132488 cites W2152804357 @default.
• W2008132488 cites W2155779568 @default.
• W2008132488 cites W2164122728 @default.
• W2008132488 cites W2165489255 @default.
• W2008132488 cites W2169694555 @default.
• W2008132488 cites W2171291743 @default.
• W2008132488 cites W2763997862 @default.
• W2008132488 cites W3098002080 @default.
• W2008132488 cites W3098086022 @default.
• W2008132488 cites W3099753903 @default.
• W2008132488 cites W3099758390 @default.
• W2008132488 cites W3100314980 @default.
• W2008132488 cites W3100514350 @default.
• W2008132488 cites W3100566534 @default.
• W2008132488 cites W3100600490 @default.
• W2008132488 cites W3101296676 @default.
• W2008132488 cites W3101646687 @default.
• W2008132488 cites W3101756647 @default.
• W2008132488 cites W3101803150 @default.
• W2008132488 cites W3102058054 @default.
• W2008132488 cites W3103071107 @default.

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