Matches in SemOpenAlex for { <https://semopenalex.org/work/W1984162005> ?p ?o ?g. }
- W1984162005 endingPage "67" @default.
- W1984162005 startingPage "67" @default.
- W1984162005 abstract "Stellar rotation is a strong function of both mass and evolutionary state. Missions such as Kepler and CoRoT provide tens of thousands of rotation periods, drawn from stellar populations that contain objects at a range of masses, ages, and evolutionary states. Given a set of reasonable starting conditions and a prescription for angular momentum loss, we address the expected range of rotation periods for cool field stellar populations (∼0.4–2.0 M☉). We find that cool stars fall into three distinct regimes in rotation. Rapid rotators with surface periods less than 10 days are either young low-mass main sequence (MS) stars, or higher mass subgiants which leave the MS with high rotation rates. Intermediate rotators (10–40 days) can be either cool MS dwarfs, suitable for gyrochronology, or crossing subgiants at a range of masses. Gyrochronology relations must therefore be applied cautiously, since there is an abundant population of subgiant contaminants. The slowest rotators, at periods greater than 40 days, are lower mass subgiants undergoing envelope expansion. We identify additional diagnostic uses of rotation periods. There exists a period–age relation for subgiants distinct from the MS period–age relations. There is also a period–radius relation that can be used as a constraint on the stellar radius, particularly in the interesting case of planet host stars. The high-mass/low-mass break in the rotation distribution on the MS persists onto the subgiant branch, and has potential as a diagnostic of stellar mass. Finally, this set of theoretical predictions can be compared to extensive datasets to motivate improved modeling." @default.
- W1984162005 created "2016-06-24" @default.
- W1984162005 creator A5058919944 @default.
- W1984162005 creator A5071573101 @default.
- W1984162005 date "2013-09-26" @default.
- W1984162005 modified "2023-10-16" @default.
- W1984162005 title "FAST STAR, SLOW STAR; OLD STAR, YOUNG STAR: SUBGIANT ROTATION AS A POPULATION AND STELLAR PHYSICS DIAGNOSTIC" @default.
- W1984162005 cites W1867591249 @default.
- W1984162005 cites W1927928721 @default.
- W1984162005 cites W1963757454 @default.
- W1984162005 cites W1963968906 @default.
- W1984162005 cites W1965024870 @default.
- W1984162005 cites W1978391636 @default.
- W1984162005 cites W1987673843 @default.
- W1984162005 cites W1992510589 @default.
- W1984162005 cites W1992730873 @default.
- W1984162005 cites W1996491041 @default.
- W1984162005 cites W2006124034 @default.
- W1984162005 cites W2011569645 @default.
- W1984162005 cites W2012578543 @default.
- W1984162005 cites W2016893051 @default.
- W1984162005 cites W2018544032 @default.
- W1984162005 cites W2023344645 @default.
- W1984162005 cites W2023675460 @default.
- W1984162005 cites W2025092105 @default.
- W1984162005 cites W2025977350 @default.
- W1984162005 cites W2036696684 @default.
- W1984162005 cites W2039706123 @default.
- W1984162005 cites W2043026411 @default.
- W1984162005 cites W2043250362 @default.
- W1984162005 cites W2048109974 @default.
- W1984162005 cites W2050212175 @default.
- W1984162005 cites W2061759127 @default.
- W1984162005 cites W2063710750 @default.
- W1984162005 cites W2064616248 @default.
- W1984162005 cites W2065472013 @default.
- W1984162005 cites W2066660495 @default.
- W1984162005 cites W2068240743 @default.
- W1984162005 cites W2069988667 @default.
- W1984162005 cites W2070240923 @default.
- W1984162005 cites W2070508637 @default.
- W1984162005 cites W2075329702 @default.
- W1984162005 cites W2077310516 @default.
- W1984162005 cites W2083158503 @default.
- W1984162005 cites W2090434735 @default.
- W1984162005 cites W2098212955 @default.
- W1984162005 cites W2098479840 @default.
- W1984162005 cites W2100714188 @default.
- W1984162005 cites W2108892540 @default.
- W1984162005 cites W2111220702 @default.
- W1984162005 cites W2113396363 @default.
- W1984162005 cites W2115636841 @default.
- W1984162005 cites W2127239784 @default.
- W1984162005 cites W2130553508 @default.
- W1984162005 cites W2136459797 @default.
- W1984162005 cites W2142350809 @default.
- W1984162005 cites W2147196428 @default.
- W1984162005 cites W2154090931 @default.
- W1984162005 cites W2161791806 @default.
- W1984162005 cites W2167549591 @default.
- W1984162005 cites W2169586648 @default.
- W1984162005 cites W2499926027 @default.
- W1984162005 cites W2554732597 @default.
- W1984162005 cites W3098643748 @default.
- W1984162005 cites W3099359742 @default.
- W1984162005 cites W3099445296 @default.
- W1984162005 cites W3099491888 @default.
- W1984162005 cites W3100231519 @default.
- W1984162005 cites W3101487936 @default.
- W1984162005 cites W3101615941 @default.
- W1984162005 cites W3104433299 @default.
- W1984162005 cites W3104523124 @default.
- W1984162005 cites W3105311284 @default.
- W1984162005 cites W3106310073 @default.
- W1984162005 cites W3106507447 @default.
- W1984162005 cites W3122771034 @default.
- W1984162005 cites W3124043341 @default.
- W1984162005 cites W4292407326 @default.
- W1984162005 cites W4293311141 @default.
- W1984162005 doi "https://doi.org/10.1088/0004-637x/776/2/67" @default.
- W1984162005 hasPublicationYear "2013" @default.
- W1984162005 type Work @default.
- W1984162005 sameAs 1984162005 @default.
- W1984162005 citedByCount "146" @default.
- W1984162005 countsByYear W19841620052013 @default.
- W1984162005 countsByYear W19841620052014 @default.
- W1984162005 countsByYear W19841620052015 @default.
- W1984162005 countsByYear W19841620052016 @default.
- W1984162005 countsByYear W19841620052017 @default.
- W1984162005 countsByYear W19841620052018 @default.
- W1984162005 countsByYear W19841620052019 @default.
- W1984162005 countsByYear W19841620052020 @default.
- W1984162005 countsByYear W19841620052021 @default.
- W1984162005 countsByYear W19841620052022 @default.
- W1984162005 countsByYear W19841620052023 @default.
- W1984162005 crossrefType "journal-article" @default.
- W1984162005 hasAuthorship W1984162005A5058919944 @default.
- W1984162005 hasAuthorship W1984162005A5071573101 @default.