Sean P. Matt, Ph.D.
Affiliations: | 2002 | University of Washington, Seattle, Seattle, WA |
Area:
Astronomy and AstrophysicsGoogle:
"Sean Matt"Mean distance: 18.3 | S | N | B | C | P |
Parents
Sign in to add mentorRobert Winglee | grad student | 2002 | University of Washington | |
(The influence of poloidal magnetic fields on astrophysical outflows.) |
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Publications
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Shoda M, Suzuki TK, Matt SP, et al. (2020) Alfvén-wave-driven Magnetic Rotator Winds from Low-mass Stars. I. Rotation Dependences of Magnetic Braking and Mass-loss Rate The Astrophysical Journal. 896: 123 |
Lehmann L, Matt S, Finley A. (2020) How much do underestimated field strengths from Zeeman-Doppler imaging affect spin-down torque estimates? The Astrophysical Journal. 894: 69 |
Amard L, Matt SP. (2020) The impact of metallicity on the evolution of the rotation and magnetic activity of Sun-like stars The Astrophysical Journal. 889: 108 |
Bastian N, Kamann S, Amard L, et al. (2020) On the origin of the bimodal rotational velocity distribution in stellar clusters: rotation on the pre-main sequence Monthly Notices of the Royal Astronomical Society. 495: 1978-1983 |
Magaudda E, Stelzer B, Covey KR, et al. (2020) Relation of X-ray activity and rotation in M dwarfs and predicted time-evolution of the X-ray luminosity Astronomy and Astrophysics. 638 |
Finley AJ, Hewitt AL, Matt SP, et al. (2019) Direct Detection of Solar Angular Momentum Loss with the Wind Spacecraft The Astrophysical Journal. 885: L30 |
Matt S, Brun A, Baraffe I, et al. (2019) Erratum: The mass-dependence of angular momentum evolution in sun-like stars (Astrophysical Journal Letters (2015)799 (L23) DOI: 10.1088/2041-8205/799/2/L23) The Astrophysical Journal. 870 |
See V, Matt SP, Finley AJ, et al. (2019) Do Non-dipolar Magnetic Fields Contribute to Spin-down Torques? The Astrophysical Journal. 886: 120 |
Finley AJ, Deshmukh S, Matt SP, et al. (2019) Solar Angular Momentum Loss Over the Past Several Millennia The Astrophysical Journal. 883: 67 |
Finley AJ, See V, Matt SP. (2019) The Effect of Magnetic Variability on Stellar Angular Momentum Loss. II. The Sun, 61 Cygni A, ϵ Eridani, ξ Bootis A, and τ Bootis A The Astrophysical Journal. 876: 44 |