FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2951061718> ?p ?o ?g. }

• W2951061718 endingPage "49" @default.
• W2951061718 startingPage "49" @default.
• W2951061718 abstract "We present large-field (4.25~$times$~3.75 deg$^2$) mapping observations toward the Galactic region centered at $l = 150arcdeg, b = 3.5arcdeg$ in the $J = 1-0$ emission line of CO isotopologues ($^{12}$CO, $^{13}$CO, and C$^{18}$O), using the 13.7 m millimeter-wavelength telescope of the Purple Mountain Observatory. Based on the $^{13}$CO observations, we reveal a filamentary cloud in the Local Arm at a velocity range of $-$0.5 to 6.5~km~s$^{-1}$. This molecular cloud contains 1 main filament and 11 sub-filaments, showing the so-called ridge-nest structure. The main filament and three sub-filaments are also detected in the C$^{18}$O line. The velocity structures of most identified filaments display continuous distribution with slight velocity gradients. The measured median excitation temperature, line width, length, width, and linear mass of the filaments are $sim$9.28~K, 0.85~km~s$^{-1}$, 7.30~pc, 0.79~pc, and 17.92~$M_sun$~pc$^{-1}$, respectively, assuming a distance of 400~pc. We find that the four filaments detected in the C$^{18}$O line are thermally supercritical, and two of them are in the virialized state, and thus tend to be gravitationally bound. We identify in total 146 $^{13}$CO clumps in the cloud, about 77$%$ of the clumps are distributed along the filaments. About 56$%$ of the virialized clumps are found to be associated with the supercritical filaments. Three young stellar object (YSO) candidates are also identified in the supercritical filaments, based on the complementary infrared (IR) data. These results indicate that the supercritical filaments, especially the virialized filaments, may contain star-forming activities." @default.
• W2951061718 created "2019-06-27" @default.
• W2951061718 creator A5012968406 @default.
• W2951061718 creator A5024917626 @default.
• W2951061718 creator A5028789695 @default.
• W2951061718 creator A5030173674 @default.
• W2951061718 creator A5033640947 @default.
• W2951061718 creator A5060310147 @default.
• W2951061718 creator A5061565884 @default.
• W2951061718 creator A5070014170 @default.
• W2951061718 date "2017-03-23" @default.
• W2951061718 modified "2023-09-27" @default.
• W2951061718 title "CO(<i>J</i>= 1–0) Observations of a Filamentary Molecular Cloud in the Galactic Region Centered at<i>l</i>= 150°,<i>b</i>= 3.°5" @default.
• W2951061718 cites W1972664573 @default.
• W2951061718 cites W1976666257 @default.
• W2951061718 cites W1979288367 @default.
• W2951061718 cites W2004485661 @default.
• W2951061718 cites W2005509839 @default.
• W2951061718 cites W2017002018 @default.
• W2951061718 cites W2017721755 @default.
• W2951061718 cites W2022845636 @default.
• W2951061718 cites W2028181754 @default.
• W2951061718 cites W2032799943 @default.
• W2951061718 cites W2043647577 @default.
• W2951061718 cites W2045096837 @default.
• W2951061718 cites W2049707893 @default.
• W2951061718 cites W2052937506 @default.
• W2951061718 cites W2054720561 @default.
• W2951061718 cites W2055506692 @default.
• W2951061718 cites W2057015676 @default.
• W2951061718 cites W2064412245 @default.
• W2951061718 cites W2074529843 @default.
• W2951061718 cites W2081287082 @default.
• W2951061718 cites W2087207733 @default.
• W2951061718 cites W2104356617 @default.
• W2951061718 cites W2119771582 @default.
• W2951061718 cites W2142220522 @default.
• W2951061718 cites W2150372924 @default.
• W2951061718 cites W2154298686 @default.
• W2951061718 cites W2156658280 @default.
• W2951061718 cites W2171603061 @default.
• W2951061718 cites W2405905990 @default.
• W2951061718 cites W2531241195 @default.
• W2951061718 cites W3099830973 @default.
• W2951061718 cites W3100364492 @default.
• W2951061718 cites W3100511326 @default.
• W2951061718 cites W3101550428 @default.
• W2951061718 cites W3102087921 @default.
• W2951061718 cites W3102263326 @default.
• W2951061718 cites W3102867215 @default.
• W2951061718 cites W3103220539 @default.
• W2951061718 cites W3103399299 @default.
• W2951061718 cites W3103653812 @default.
• W2951061718 cites W3103936180 @default.
• W2951061718 cites W3104423841 @default.
• W2951061718 cites W3105922414 @default.
• W2951061718 cites W3121592479 @default.
• W2951061718 cites W3122470830 @default.
• W2951061718 cites W4289815540 @default.
• W2951061718 cites W4293107329 @default.
• W2951061718 cites W4308645194 @default.
• W2951061718 doi "https://doi.org/10.3847/1538-4357/aa6443" @default.
• W2951061718 hasPublicationYear "2017" @default.
• W2951061718 type Work @default.
• W2951061718 sameAs 2951061718 @default.
• W2951061718 citedByCount "15" @default.
• W2951061718 countsByYear W29510617182017 @default.
• W2951061718 countsByYear W29510617182018 @default.
• W2951061718 countsByYear W29510617182019 @default.
• W2951061718 countsByYear W29510617182020 @default.
• W2951061718 countsByYear W29510617182021 @default.
• W2951061718 countsByYear W29510617182022 @default.
• W2951061718 countsByYear W29510617182023 @default.
• W2951061718 crossrefType "journal-article" @default.
• W2951061718 hasAuthorship W2951061718A5012968406 @default.
• W2951061718 hasAuthorship W2951061718A5024917626 @default.
• W2951061718 hasAuthorship W2951061718A5028789695 @default.
• W2951061718 hasAuthorship W2951061718A5030173674 @default.
• W2951061718 hasAuthorship W2951061718A5033640947 @default.
• W2951061718 hasAuthorship W2951061718A5060310147 @default.
• W2951061718 hasAuthorship W2951061718A5061565884 @default.
• W2951061718 hasAuthorship W2951061718A5070014170 @default.
• W2951061718 hasBestOaLocation W29510617181 @default.
• W2951061718 hasConcept C121332964 @default.
• W2951061718 hasConcept C125857072 @default.
• W2951061718 hasConcept C1276947 @default.
• W2951061718 hasConcept C13934619 @default.
• W2951061718 hasConcept C14228908 @default.
• W2951061718 hasConcept C150846664 @default.
• W2951061718 hasConcept C198352243 @default.
• W2951061718 hasConcept C23254167 @default.
• W2951061718 hasConcept C2524010 @default.
• W2951061718 hasConcept C33923547 @default.
• W2951061718 hasConcept C44870925 @default.
• W2951061718 hasConcept C4839761 @default.
• W2951061718 hasConcept C54355233 @default.
• W2951061718 hasConcept C86021447 @default.
• W2951061718 hasConcept C86803240 @default.

• next