FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3145619034> ?p ?o ?g. }

• W3145619034 endingPage "207" @default.
• W3145619034 startingPage "199" @default.
• W3145619034 abstract "ABSTRACT We estimate the solar peculiar velocities and Oort constants using a sample of 5627 A-type stars with $dlt 0.6, rm kpc$ and $|z|lt 0.1, rm kpc$, selected from the LAMOST (Large Sky Area Multi-Object Fiber Spectroscopic Telescope) surveys. The radial and tangential velocities of these A-type stars are fitted by using a non-axisymmetric model. The best-fitting result yields the solar peculiar velocities $(U_odot ,V_odot ,W_odot)=(11.69pm 0.68, 10.16pm 0.51, 7.67pm 0.10), rm km, s^{-1}$ and Oort constants $A=16.31pm 0.89, rm km, s^{-1}, kpc^{-1}$, $B=-11.99pm 0.79, rm km, s^{-1}, kpc^{-1}$, $C=-3.10pm 0.48, rm km, s^{-1}, kpc^{-1}$, and $K=-1.25pm 1.04, rm km, s^{-1}, kpc^{-1}$. $|K+C|gt 4, rm km, s^{-1}, kpc^{-1}$ means that there is a radial velocity gradient in the extended local disc, implying that the local disc is in a non-asymmetric potential. Using the derived Oort constants, we derive the local angular velocity $Omega , {approx }, A-B=28.30pm 1.19, rm km, s^{-1}, kpc^{-1}$. By using A-type star sample of different volumes, we further try to evaluate the impacts of the ridge pattern in the R–Vϕ plane on constraining the solar motions and Oort constants. As the volume becomes larger towards the anticentre direction, the values of A and B become larger (implying a steeper slope of the local rotation curve) and the value of V⊙ becomes smaller probably caused by the ridge structure and its signal increasing with distance." @default.
• W3145619034 created "2021-04-13" @default.
• W3145619034 creator A5006815516 @default.
• W3145619034 creator A5007758223 @default.
• W3145619034 creator A5020241207 @default.
• W3145619034 creator A5022458256 @default.
• W3145619034 creator A5071163972 @default.
• W3145619034 creator A5087434579 @default.
• W3145619034 date "2021-03-25" @default.
• W3145619034 modified "2023-10-16" @default.
• W3145619034 title "Local stellar kinematics and Oort constants from the LAMOST A-type stars" @default.
• W3145619034 cites W1834459731 @default.
• W3145619034 cites W1967016106 @default.
• W3145619034 cites W1979379324 @default.
• W3145619034 cites W1992773509 @default.
• W3145619034 cites W1998084400 @default.
• W3145619034 cites W2008200089 @default.
• W3145619034 cites W2011490256 @default.
• W3145619034 cites W2028070372 @default.
• W3145619034 cites W2038116318 @default.
• W3145619034 cites W2047258477 @default.
• W3145619034 cites W2052937506 @default.
• W3145619034 cites W2057634812 @default.
• W3145619034 cites W2072461515 @default.
• W3145619034 cites W2109878337 @default.
• W3145619034 cites W2111817932 @default.
• W3145619034 cites W2121480729 @default.
• W3145619034 cites W2142220522 @default.
• W3145619034 cites W2155488926 @default.
• W3145619034 cites W2170011509 @default.
• W3145619034 cites W2341946664 @default.
• W3145619034 cites W2540643402 @default.
• W3145619034 cites W2578206578 @default.
• W3145619034 cites W2593734852 @default.
• W3145619034 cites W2740236269 @default.
• W3145619034 cites W2780502734 @default.
• W3145619034 cites W2798336535 @default.
• W3145619034 cites W2799258675 @default.
• W3145619034 cites W2834751994 @default.
• W3145619034 cites W2890840461 @default.
• W3145619034 cites W2912242616 @default.
• W3145619034 cites W2915081804 @default.
• W3145619034 cites W2916546127 @default.
• W3145619034 cites W2949380767 @default.
• W3145619034 cites W3043649483 @default.
• W3145619034 cites W3080245202 @default.
• W3145619034 cites W3100127245 @default.
• W3145619034 cites W3100330265 @default.
• W3145619034 cites W3100380585 @default.
• W3145619034 cites W3102784118 @default.
• W3145619034 cites W3103263672 @default.
• W3145619034 cites W3105791279 @default.
• W3145619034 cites W3106003303 @default.
• W3145619034 cites W3122336616 @default.
• W3145619034 cites W3122591886 @default.
• W3145619034 cites W3124275756 @default.
• W3145619034 cites W3125696588 @default.
• W3145619034 cites W4229757247 @default.
• W3145619034 doi "https://doi.org/10.1093/mnras/stab848" @default.
• W3145619034 hasPublicationYear "2021" @default.
• W3145619034 type Work @default.
• W3145619034 sameAs 3145619034 @default.
• W3145619034 citedByCount "14" @default.
• W3145619034 countsByYear W31456190342021 @default.
• W3145619034 countsByYear W31456190342022 @default.
• W3145619034 countsByYear W31456190342023 @default.
• W3145619034 crossrefType "journal-article" @default.
• W3145619034 hasAuthorship W3145619034A5006815516 @default.
• W3145619034 hasAuthorship W3145619034A5007758223 @default.
• W3145619034 hasAuthorship W3145619034A5020241207 @default.
• W3145619034 hasAuthorship W3145619034A5022458256 @default.
• W3145619034 hasAuthorship W3145619034A5071163972 @default.
• W3145619034 hasAuthorship W3145619034A5087434579 @default.
• W3145619034 hasBestOaLocation W31456190342 @default.
• W3145619034 hasConcept C121332964 @default.
• W3145619034 hasConcept C150846664 @default.
• W3145619034 hasConcept C18903297 @default.
• W3145619034 hasConcept C2777299769 @default.
• W3145619034 hasConcept C2778139282 @default.
• W3145619034 hasConcept C2780897414 @default.
• W3145619034 hasConcept C41074950 @default.
• W3145619034 hasConcept C44870925 @default.
• W3145619034 hasConcept C86803240 @default.
• W3145619034 hasConceptScore W3145619034C121332964 @default.
• W3145619034 hasConceptScore W3145619034C150846664 @default.
• W3145619034 hasConceptScore W3145619034C18903297 @default.
• W3145619034 hasConceptScore W3145619034C2777299769 @default.
• W3145619034 hasConceptScore W3145619034C2778139282 @default.
• W3145619034 hasConceptScore W3145619034C2780897414 @default.
• W3145619034 hasConceptScore W3145619034C41074950 @default.
• W3145619034 hasConceptScore W3145619034C44870925 @default.
• W3145619034 hasConceptScore W3145619034C86803240 @default.
• W3145619034 hasFunder F4320321001 @default.
• W3145619034 hasFunder F4320324731 @default.
• W3145619034 hasFunder F4320335777 @default.
• W3145619034 hasIssue "1" @default.
• W3145619034 hasLocation W31456190341 @default.
• W3145619034 hasLocation W31456190342 @default.

• next