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• W3176383756 abstract "We present a statistical study of the filamentary structure orientation inthe CO emission observations obtained in the Milky Way Imaging Scroll Painting(MWISP) survey in the range $25.8deg < l < 49.7deg$, $|b| leq 1.25deg$, and$-100 < v_{rm LSR} < 135$ km/s. We found that most of the filamentarystructures in the $^{12}$CO and $^{13}$CO emission do not show a globalpreferential orientation either parallel or perpendicular to the Galacticplane. However, we found ranges in Galactic longitude and radial velocity wherethe $^{12}$CO and $^{13}$CO filamentary structures are parallel to the Galacticplane. These preferential orientations are different from those found for theHI emission. We consider this an indication that the molecular structures donot simply inherit these properties from parental atomic clouds. Instead, theyare shaped by local physical conditions, such as stellar feedback, magneticfields, and Galactic spiral shocks." @default.
• W3176383756 created "2021-07-05" @default.
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• W3176383756 date "2021-06-24" @default.
• W3176383756 modified "2023-09-27" @default.
• W3176383756 title "The filamentary structures in the CO emission toward the Milky Way disk" @default.
• W3176383756 hasPublicationYear "2021" @default.
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