Search Results - "Metcalfe, Travis S."
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Magnetic Evolution and the Disappearance of Sun-Like Activity Cycles
Published in Solar physics (01-09-2017)“…After decades of effort, the solar activity cycle is exceptionally well characterized, but it remains poorly understood. Pioneering work at the Mount Wilson…”
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Evolution of Co-existing Long and Short Period Stellar Activity Cycles
Published in The Astrophysical journal (10-08-2017)“…The magnetic activity of the Sun becomes stronger and weaker over roughly an 11 year cycle, modulating the radiation and charged particle environment…”
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3
Understanding the Limitations of Gyrochronology for Old Field Stars
Published in The Astrophysical journal (20-01-2019)“…Nearly half a century has passed since the initial indications that stellar rotation slows while chromospheric activity weakens with a power-law dependence on…”
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Weakened magnetic braking as the origin of anomalously rapid rotation in old field stars
Published in Nature (London) (14-01-2016)“…The age of a young to middle-aged star can be determined from how quickly or slowly it rotates, but the relationship breaks down for old stars; models now show…”
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CoRoT Reveals a Magnetic Activity Cycle in a Sun-Like Star
Published in Science (American Association for the Advancement of Science) (27-08-2010)“…The 11-year activity cycle of the Sun is a consequence of a dynamo process occurring beneath its surface. We analyzed photometric data obtained by the CoRoT…”
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The Origin of Weakened Magnetic Braking in Old Solar Analogs
Published in Astrophysical journal. Letters (01-07-2022)“…Abstract The rotation rates of main-sequence stars slow over time as they gradually lose angular momentum to their magnetized stellar winds. The rate of…”
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The Influence of Metallicity on Stellar Differential Rotation and Magnetic Activity
Published in The Astrophysical journal (01-01-2018)“…Observations of Sun-like stars over the past half-century have improved our understanding of how magnetic dynamos, like that responsible for the 11 yr solar…”
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Stellar Cruise Control: Weakened Magnetic Braking Leads to Sustained Rapid Rotation of Old Stars
Published in The Astrophysical journal (01-02-2024)“…Abstract Despite a growing sample of precisely measured stellar rotation periods and ages, the strength of magnetic braking and the degree of departure from…”
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TESS Asteroseismology of β Hydri: A Subgiant with a Born-again Dynamo
Published in The Astrophysical journal (01-10-2024)“…Abstract The solar-type subgiant β Hyi has long been studied as an old analog of the Sun. Although the rotation period has never been measured directly, it was…”
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A New Asteroseismic Kepler Benchmark Constrains the Onset of Weakened Magnetic Braking in Mature Sun-like Stars
Published in The Astrophysical journal (01-08-2024)“…Abstract Stellar spin down is a critical yet poorly understood component of stellar evolution. In particular, results from the Kepler Mission imply that mature…”
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Constraints on Magnetic Braking from the G8 Dwarf Stars 61 UMa and τ Cet
Published in Astrophysical journal. Letters (01-05-2023)“…Abstract During the first half of their main-sequence lifetimes, stars rapidly lose angular momentum to their magnetized winds, a process known as magnetic…”
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ASTEROSEISMIC ESTIMATE OF HELIUM ABUNDANCE OF A SOLAR ANALOG BINARY SYSTEM
Published in The Astrophysical journal (01-08-2014)“…16 Cyg A and B are among the brightest stars observed by Kepler. What makes these stars more interesting is that they are solar analogs. 16 Cyg A and B exhibit…”
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Weakened Magnetic Braking in the Exoplanet Host Star 51 Peg
Published in Astrophysical journal. Letters (01-01-2024)“…Abstract The consistently low activity level of the old solar analog 51 Peg not only facilitated the discovery of the first hot Jupiter, but also led to the…”
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Asteroseismology and Spectropolarimetry of the Exoplanet Host Star λ Serpentis
Published in The Astronomical journal (01-10-2023)“…Abstract The bright star λ Ser hosts a hot Neptune with a minimum mass of 13.6 M ⊕ and a 15.5 day orbit. It also appears to be a solar analog, with a mean…”
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Stellar Activity Cycles
Published in Space science reviews (01-10-2023)“…The magnetic field of the Sun is generated by internal dynamo process with a cyclic period of 11 years or a 22 year magnetic cycle. The signatures of the Sun’s…”
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Scaling and Evolution of Stellar Magnetic Activity
Published in Space science reviews (01-12-2023)“…Magnetic activity is a ubiquitous feature of stars with convective outer layers, with implications from stellar evolution to planetary atmospheres…”
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SUN-LIKE MAGNETIC CYCLES IN THE RAPIDLY ROTATING YOUNG SOLAR ANALOG HD 30495
Published in The Astrophysical journal (10-10-2015)“…ABSTRACT A growing body of evidence suggests that multiple dynamo mechanisms can drive magnetic variability on different timescales, not only in the Sun but…”
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Stellar Spin-Orbit Misalignment in a Multiplanet System
Published in Science (American Association for the Advancement of Science) (18-10-2013)“…Stars hosting hot Jupiters are often observed to have high obliquities, whereas stars with multiple coplanar planets have been seen to have low obliquities…”
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Seismic inference of 57 stars using full-length Kepler data sets
Published in EPJ Web of Conferences (01-01-2017)“…We present stellar properties of 57 stars from a seismic inference using full-length data sets from Kepler (mass, age, radius, distances). These stars comprise…”
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Brightness Fluctuation Spectra of Sun-like Stars. I. The Mid-frequency Continuum
Published in The Astrophysical journal (01-08-2021)“…Abstract We analyze space-based time-series photometry of Sun-like stars, mostly in the Pleiades, but also field stars and the Sun itself. We focus on…”
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