FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3100563152> ?p ?o ?g. }

• W3100563152 endingPage "117" @default.
• W3100563152 startingPage "117" @default.
• W3100563152 abstract "We used the Green Bank Telescope to detect molecular lines observed toward Mid-Infrared (MIR) bubbles N62, N65, N90, and N117. The bubbles were selected from Watson et al. (2016) who detected non-Gaussian CS (1-0) emission lines toward the bubbles. Two of the bubbles are adjacent to infrared dark clouds (IRDCs); we examined these sources for evidence of interaction between the bubble rim and IRDC. The other two bubbles contain YSOs interior to the bubble rim; in these sources we observed the gas near the YSOs. We detect CS (1-0) emission toward all of the sources, and in several pointings the CS emission shows non-Gaussian line shapes. HC$_3$N (5-4), C$^{34}$S (1-0), CH$_3$OH (1-0), and SiO (v=0) (1-0) were also detected in some pointings. We calculate column densities and abundances for the detected molecules. We compare the velocity of optically-thick CS emission with the velocity of the other, optically thin lines to look for evidence of infall. We find that even in pointings with non-Gaussian CS emission, our detections do not support an infall model. We interpret the kinematics of the gas in N62, N65, and N117 as likely evidence of multiple clouds along the line of sight moving at slightly offset velocities. We do not detect evidence of bubble rims interacting with IRDCs in N62 or N90. The gas interior to bubbles appears more disrupted than the gas in the IRDCs. N65 shows significantly stronger emission lines than the other sources, as well as the most complicated non-Gaussian line shapes." @default.
• W3100563152 created "2020-11-23" @default.
• W3100563152 creator A5007195034 @default.
• W3100563152 creator A5013034544 @default.
• W3100563152 creator A5036521335 @default.
• W3100563152 creator A5045033761 @default.
• W3100563152 creator A5068993900 @default.
• W3100563152 date "2018-07-11" @default.
• W3100563152 modified "2023-10-18" @default.
• W3100563152 title "A Molecular Line Investigation of the Interaction between Mid-infrared Bubbles and the Interstellar Medium" @default.
• W3100563152 cites W1926942421 @default.
• W3100563152 cites W1966062726 @default.
• W3100563152 cites W1973143959 @default.
• W3100563152 cites W1975265102 @default.
• W3100563152 cites W1975338557 @default.
• W3100563152 cites W1978764303 @default.
• W3100563152 cites W1982817299 @default.
• W3100563152 cites W1988977509 @default.
• W3100563152 cites W1989282130 @default.
• W3100563152 cites W1990209086 @default.
• W3100563152 cites W1990841834 @default.
• W3100563152 cites W1997129313 @default.
• W3100563152 cites W2000616991 @default.
• W3100563152 cites W2006521339 @default.
• W3100563152 cites W2014188465 @default.
• W3100563152 cites W2028186818 @default.
• W3100563152 cites W2032417424 @default.
• W3100563152 cites W2033725176 @default.
• W3100563152 cites W2039960576 @default.
• W3100563152 cites W2041690704 @default.
• W3100563152 cites W2041730224 @default.
• W3100563152 cites W2078875725 @default.
• W3100563152 cites W2086764113 @default.
• W3100563152 cites W2088885427 @default.
• W3100563152 cites W2093342937 @default.
• W3100563152 cites W2093858980 @default.
• W3100563152 cites W2108064551 @default.
• W3100563152 cites W2119967804 @default.
• W3100563152 cites W2121018712 @default.
• W3100563152 cites W2121659150 @default.
• W3100563152 cites W2130283602 @default.
• W3100563152 cites W2141099472 @default.
• W3100563152 cites W2142220522 @default.
• W3100563152 cites W2147764886 @default.
• W3100563152 cites W2150115749 @default.
• W3100563152 cites W2157253005 @default.
• W3100563152 cites W2159407551 @default.
• W3100563152 cites W2286500479 @default.
• W3100563152 cites W2341522232 @default.
• W3100563152 cites W3000746797 @default.
• W3100563152 cites W3099127675 @default.
• W3100563152 cites W3100847552 @default.
• W3100563152 cites W3102344868 @default.
• W3100563152 cites W3103020916 @default.
• W3100563152 cites W3103097675 @default.
• W3100563152 cites W3104452397 @default.
• W3100563152 cites W3104556830 @default.
• W3100563152 cites W3106007949 @default.
• W3100563152 cites W3106363423 @default.
• W3100563152 cites W3121726213 @default.
• W3100563152 cites W4232656021 @default.
• W3100563152 cites W4293185728 @default.
• W3100563152 doi "https://doi.org/10.3847/1538-4357/aac5fa" @default.
• W3100563152 hasPublicationYear "2018" @default.
• W3100563152 type Work @default.
• W3100563152 sameAs 3100563152 @default.
• W3100563152 citedByCount "2" @default.
• W3100563152 countsByYear W31005631522019 @default.
• W3100563152 countsByYear W31005631522021 @default.
• W3100563152 crossrefType "journal-article" @default.
• W3100563152 hasAuthorship W3100563152A5007195034 @default.
• W3100563152 hasAuthorship W3100563152A5013034544 @default.
• W3100563152 hasAuthorship W3100563152A5036521335 @default.
• W3100563152 hasAuthorship W3100563152A5045033761 @default.
• W3100563152 hasAuthorship W3100563152A5068993900 @default.
• W3100563152 hasBestOaLocation W31005631521 @default.
• W3100563152 hasConcept C121332964 @default.
• W3100563152 hasConcept C125857072 @default.
• W3100563152 hasConcept C1276947 @default.
• W3100563152 hasConcept C157915830 @default.
• W3100563152 hasConcept C158355884 @default.
• W3100563152 hasConcept C196939603 @default.
• W3100563152 hasConcept C198352243 @default.
• W3100563152 hasConcept C23254167 @default.
• W3100563152 hasConcept C2524010 @default.
• W3100563152 hasConcept C2780928442 @default.
• W3100563152 hasConcept C33923547 @default.
• W3100563152 hasConcept C44870925 @default.
• W3100563152 hasConcept C4839761 @default.
• W3100563152 hasConcept C57879066 @default.
• W3100563152 hasConcept C96141758 @default.
• W3100563152 hasConcept C98444146 @default.
• W3100563152 hasConceptScore W3100563152C121332964 @default.
• W3100563152 hasConceptScore W3100563152C125857072 @default.
• W3100563152 hasConceptScore W3100563152C1276947 @default.
• W3100563152 hasConceptScore W3100563152C157915830 @default.
• W3100563152 hasConceptScore W3100563152C158355884 @default.
• W3100563152 hasConceptScore W3100563152C196939603 @default.

• next