Matches in SemOpenAlex for { <https://semopenalex.org/work/W4292383610> ?p ?o ?g. }
- W4292383610 endingPage "104" @default.
- W4292383610 startingPage "104" @default.
- W4292383610 abstract "Abstract We present a study of the relationship between Galactic kinematics, flare rates, chromospheric activity, and rotation periods for a volume-complete, nearly all-sky sample of 219 single stars within 15 pc and with masses between 0.1 and 0.3 M ⊙ observed during the primary mission of TESS. We find all stars consistent with a common value of α = 1.984 ± 0.019 for the exponent of the flare frequency distribution. Using our measured stellar radial velocities and Gaia astrometry, we determine Galactic UVW space motions. We find 78% of stars are members of the Galactic thin disk, 7% belong to the thick disk, and for the remaining 15% we cannot confidently assign membership to either component. If we assume star formation has been constant in the thin disk for the past 8 Gyr, then based on the fraction that we observe to be active, we estimate the average age at which these stars transition from the saturated to the unsaturated flaring regime to be 2.4 ± 0.3 Gyr. This is consistent with the ages that we assign from Galactic kinematics: we find that stars with rotation period P rot < 10 days have an age of 2.0 ± 1.2 Gyr, stars with 10 days < P rot ≤ 90 days have an age of 5.6 ± 2.7 Gyr, and stars with P rot > 90 days have an age of 12.9 ± 3.5 Gyr. We find that the average age of stars with P rot < 10 days increases with decreasing stellar mass from 0.6 ± 0.3 Gyr (0.2–0.3 M ⊙ ) to 2.3 ± 1.3 Gyr (0.1–0.2 M ⊙ )." @default.
- W4292383610 created "2022-08-20" @default.
- W4292383610 creator A5027191191 @default.
- W4292383610 creator A5049263167 @default.
- W4292383610 creator A5061327811 @default.
- W4292383610 creator A5082240598 @default.
- W4292383610 date "2022-08-01" @default.
- W4292383610 modified "2023-10-14" @default.
- W4292383610 title "Galactic Kinematics and Observed Flare Rates of a Volume-complete Sample of Mid-to-late M Dwarfs: Constraints on the History of the Stellar Radiation Environment of Planets Orbiting Low-mass Stars" @default.
- W4292383610 cites W1644709875 @default.
- W4292383610 cites W1970076709 @default.
- W4292383610 cites W1978334384 @default.
- W4292383610 cites W1987581036 @default.
- W4292383610 cites W1991823040 @default.
- W4292383610 cites W1993489619 @default.
- W4292383610 cites W1997087322 @default.
- W4292383610 cites W2015258598 @default.
- W4292383610 cites W2016734711 @default.
- W4292383610 cites W2018270005 @default.
- W4292383610 cites W2022113292 @default.
- W4292383610 cites W2022907109 @default.
- W4292383610 cites W2035525551 @default.
- W4292383610 cites W2046154624 @default.
- W4292383610 cites W2049128673 @default.
- W4292383610 cites W2060147469 @default.
- W4292383610 cites W2064024165 @default.
- W4292383610 cites W2064945068 @default.
- W4292383610 cites W2067530731 @default.
- W4292383610 cites W2068032877 @default.
- W4292383610 cites W2085677506 @default.
- W4292383610 cites W2098479840 @default.
- W4292383610 cites W2120663217 @default.
- W4292383610 cites W2121480729 @default.
- W4292383610 cites W2127400668 @default.
- W4292383610 cites W2135625048 @default.
- W4292383610 cites W2138283621 @default.
- W4292383610 cites W2142350809 @default.
- W4292383610 cites W2160983683 @default.
- W4292383610 cites W2170011509 @default.
- W4292383610 cites W2217402295 @default.
- W4292383610 cites W2261573924 @default.
- W4292383610 cites W2463543304 @default.
- W4292383610 cites W2517381349 @default.
- W4292383610 cites W2565396336 @default.
- W4292383610 cites W2605851178 @default.
- W4292383610 cites W2755914372 @default.
- W4292383610 cites W2767848202 @default.
- W4292383610 cites W2775275747 @default.
- W4292383610 cites W2796140279 @default.
- W4292383610 cites W2798336535 @default.
- W4292383610 cites W2811304894 @default.
- W4292383610 cites W2888532099 @default.
- W4292383610 cites W2891724451 @default.
- W4292383610 cites W2896395878 @default.
- W4292383610 cites W2899342105 @default.
- W4292383610 cites W2907947108 @default.
- W4292383610 cites W2936291834 @default.
- W4292383610 cites W2963273354 @default.
- W4292383610 cites W2983581670 @default.
- W4292383610 cites W3028428798 @default.
- W4292383610 cites W3045312528 @default.
- W4292383610 cites W3088050931 @default.
- W4292383610 cites W3090131379 @default.
- W4292383610 cites W3093865753 @default.
- W4292383610 cites W3098211107 @default.
- W4292383610 cites W3099290857 @default.
- W4292383610 cites W3099348412 @default.
- W4292383610 cites W3099447803 @default.
- W4292383610 cites W3099715163 @default.
- W4292383610 cites W3099890891 @default.
- W4292383610 cites W3100484086 @default.
- W4292383610 cites W3101458401 @default.
- W4292383610 cites W3101487936 @default.
- W4292383610 cites W3101509191 @default.
- W4292383610 cites W3102014803 @default.
- W4292383610 cites W3102544449 @default.
- W4292383610 cites W3102626476 @default.
- W4292383610 cites W3102933789 @default.
- W4292383610 cites W3103895524 @default.
- W4292383610 cites W3103923294 @default.
- W4292383610 cites W3103991994 @default.
- W4292383610 cites W3104075023 @default.
- W4292383610 cites W3104075812 @default.
- W4292383610 cites W3104153708 @default.
- W4292383610 cites W3105653201 @default.
- W4292383610 cites W3105742026 @default.
- W4292383610 cites W3106177778 @default.
- W4292383610 cites W3106218727 @default.
- W4292383610 cites W3117122681 @default.
- W4292383610 cites W3124390133 @default.
- W4292383610 cites W3124674373 @default.
- W4292383610 cites W3125167775 @default.
- W4292383610 cites W3137059541 @default.
- W4292383610 cites W3204370820 @default.
- W4292383610 cites W4213056411 @default.
- W4292383610 cites W4221122816 @default.
- W4292383610 cites W4225727721 @default.
- W4292383610 cites W4232124878 @default.