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Sean P. Matt

Researcher at University of Exeter

Publications -  145
Citations -  5257

Sean P. Matt is an academic researcher from University of Exeter. The author has contributed to research in topics: Stars & Angular momentum. The author has an hindex of 39, co-authored 141 publications receiving 4707 citations. Previous affiliations of Sean P. Matt include McMaster University & University of Virginia.

Papers
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Journal ArticleDOI

The disk-bearing young star IM Lupi - X-ray properties and limits on accretion

Hans Moritz Günther, +7 more
- 01 Sep 2010 - 
TL;DR: In this paper, a Chandra grating spectrum and additional XMM-Newton data of IM Lup and accompanying optical spectra were used to test whether these features correlate with accretion or the presence of a disk.
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The Nature of Stellar Winds in the Star-Disk Interaction

Sean P. Matt, +1 more
- 02 Jul 2007 - 
TL;DR: In this paper, the mass loss rate from accretion-powered coronal winds of T Tauri stars was analyzed and an upper limit was established for mass loss rates of 1e-11 solar masses per year.
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Velocity asymmetries in YSO jets: Intrinsic and extrinsic mechanisms

Titos Matsakos, +9 more
- 04 Aug 2012 - 
TL;DR: In this paper, the authors investigate the origin of asymmetric YSO jet velocities and explore the effects of a potential difference in the pressure of the environment, as a consequence of the non-uniform density distribution of molecular clouds.
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Relation of X-ray activity and rotation in M dwarfs and predicted time-evolution of the X-ray luminosity

E. Magaudda, +5 more
- 06 Apr 2020 - 
TL;DR: In this article, a sample of 14 M dwarf stars observed with XMM-Newton and Chandra, for which they also computed rotational periods from Kepler Two-Wheel (K2) Mission light curves, were used to provide the largest uniform sample of M dwarfs (302 stars) for X-ray activity and rotation studies to date.
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Velocity asymmetries in young stellar object jets - Intrinsic and extrinsic mechanisms

Titos Matsakos, +9 more
- 01 Sep 2012 - 
TL;DR: In this article, the authors investigate the origin of asymmetric YSO jet velocities, and investigate the efficiency of two candidate mechanisms, one based on the intrinsic properties of the system and the other on the role of the external medium.