FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2137777144> ?p ?o ?g. }

• W2137777144 endingPage "1099" @default.
• W2137777144 startingPage "1079" @default.
• W2137777144 abstract "We present model spectral energy distributions, colors, polarization, and images for an evolutionary sequence of a low-mass protostar from the early collapse stage (Class 0) to the remnant disk stage (Class III). We find a substantial overlap in colors and SEDs between protostars embedded in envelopes (Class 0-I) and T Tauri disks (Class II), especially at mid-IR wavelengths. Edge-on Class I-II sources show double-peaked spectral energy distributions, with a short-wavelength hump due to scattered light and the long-wavelength hump due to thermal emission. These are the bluest sources in mid-IR color-color diagrams. Since Class 0 and I sources are diffuse, the size of the aperture over which fluxes are integrated has a substantial effect on the computed colors, with larger aperture results showing significantly bluer colors. This causes overlap in color-color diagrams between all evolutionary states, especially in the mid-IR. However the near-IR polarization of the Class 0 sources is much higher than the Class I-II sources, providing a means to separate these evolutionary states. We varied the grain properties in the circumstellar envelope, allowing for larger grains in the disk midplane and smaller in the envelope. We find that grain growth in disks of Class I sources can be detected at wavelengths greater than 100 $mu$m. Our image calculations predict that the diffuse emission from edge-on Class I and II sources should be detectable in the mid-IR with the Space Infrared Telescope Facility (SIRTF) in nearby star forming regions (out to several hundred parsecs)." @default.
• W2137777144 created "2016-06-24" @default.
• W2137777144 creator A5011159548 @default.
• W2137777144 creator A5020379510 @default.
• W2137777144 creator A5022336070 @default.
• W2137777144 creator A5061765401 @default.
• W2137777144 date "2003-12-01" @default.
• W2137777144 modified "2023-10-17" @default.
• W2137777144 title "Two‐dimensional Radiative Transfer in Protostellar Envelopes. II. An Evolutionary Sequence" @default.
• W2137777144 cites W1619634704 @default.
• W2137777144 cites W1666704755 @default.
• W2137777144 cites W1669866709 @default.
• W2137777144 cites W1964080181 @default.
• W2137777144 cites W1965187830 @default.
• W2137777144 cites W1967489937 @default.
• W2137777144 cites W1978263165 @default.
• W2137777144 cites W1980461186 @default.
• W2137777144 cites W1983103860 @default.
• W2137777144 cites W1983270357 @default.
• W2137777144 cites W1983509013 @default.
• W2137777144 cites W1986287730 @default.
• W2137777144 cites W1986455163 @default.
• W2137777144 cites W1987025403 @default.
• W2137777144 cites W1991238839 @default.
• W2137777144 cites W1996878024 @default.
• W2137777144 cites W1998527497 @default.
• W2137777144 cites W1998749206 @default.
• W2137777144 cites W1999263013 @default.
• W2137777144 cites W2003496651 @default.
• W2137777144 cites W2014488392 @default.
• W2137777144 cites W2016573758 @default.
• W2137777144 cites W2018760366 @default.
• W2137777144 cites W2020114314 @default.
• W2137777144 cites W2033486535 @default.
• W2137777144 cites W2042484924 @default.
• W2137777144 cites W2047457888 @default.
• W2137777144 cites W2052417193 @default.
• W2137777144 cites W2056080366 @default.
• W2137777144 cites W2058514986 @default.
• W2137777144 cites W2064859795 @default.
• W2137777144 cites W2065061110 @default.
• W2137777144 cites W2065708381 @default.
• W2137777144 cites W2071718793 @default.
• W2137777144 cites W2071956358 @default.
• W2137777144 cites W2074299830 @default.
• W2137777144 cites W2075105883 @default.
• W2137777144 cites W2081299122 @default.
• W2137777144 cites W2088318679 @default.
• W2137777144 cites W2094592974 @default.
• W2137777144 cites W2096594817 @default.
• W2137777144 cites W2099559854 @default.
• W2137777144 cites W2100868042 @default.
• W2137777144 cites W2103681340 @default.
• W2137777144 cites W2115932981 @default.
• W2137777144 cites W2119680152 @default.
• W2137777144 cites W2120469564 @default.
• W2137777144 cites W2140551581 @default.
• W2137777144 cites W2145230401 @default.
• W2137777144 cites W2159178210 @default.
• W2137777144 cites W2167635287 @default.
• W2137777144 cites W2172028936 @default.
• W2137777144 cites W2465945632 @default.
• W2137777144 cites W3091676088 @default.
• W2137777144 cites W3098902607 @default.
• W2137777144 cites W3100314980 @default.
• W2137777144 cites W3101158613 @default.
• W2137777144 cites W3103165842 @default.
• W2137777144 cites W3103722999 @default.
• W2137777144 cites W343244306 @default.
• W2137777144 cites W4243876973 @default.
• W2137777144 doi "https://doi.org/10.1086/379068" @default.
• W2137777144 hasPublicationYear "2003" @default.
• W2137777144 type Work @default.
• W2137777144 sameAs 2137777144 @default.
• W2137777144 citedByCount "364" @default.
• W2137777144 countsByYear W21377771442012 @default.
• W2137777144 countsByYear W21377771442013 @default.
• W2137777144 countsByYear W21377771442014 @default.
• W2137777144 countsByYear W21377771442015 @default.
• W2137777144 countsByYear W21377771442016 @default.
• W2137777144 countsByYear W21377771442017 @default.
• W2137777144 countsByYear W21377771442018 @default.
• W2137777144 countsByYear W21377771442019 @default.
• W2137777144 countsByYear W21377771442020 @default.
• W2137777144 countsByYear W21377771442021 @default.
• W2137777144 countsByYear W21377771442022 @default.
• W2137777144 countsByYear W21377771442023 @default.
• W2137777144 crossrefType "journal-article" @default.
• W2137777144 hasAuthorship W2137777144A5011159548 @default.
• W2137777144 hasAuthorship W2137777144A5020379510 @default.
• W2137777144 hasAuthorship W2137777144A5022336070 @default.
• W2137777144 hasAuthorship W2137777144A5061765401 @default.
• W2137777144 hasBestOaLocation W21377771441 @default.
• W2137777144 hasConcept C120665830 @default.
• W2137777144 hasConcept C121332964 @default.
• W2137777144 hasConcept C125857072 @default.
• W2137777144 hasConcept C1276947 @default.
• W2137777144 hasConcept C147789679 @default.

• next