J
Jeffrey L. Linsky
Researcher at University of Colorado Boulder
Publications - 514
Citations - 23061
Jeffrey L. Linsky is an academic researcher from University of Colorado Boulder. The author has contributed to research in topics: Stars & Interstellar medium. The author has an hindex of 83, co-authored 506 publications receiving 21746 citations. Previous affiliations of Jeffrey L. Linsky include National Institute of Standards and Technology & Association of Universities for Research in Astronomy.
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Journal ArticleDOI
Relations among stellar X-ray emission observed from Einstein, stellar rotation and bolometric luminosity
TL;DR: The correlation between observed stellar X-ray luminosities and projected rotational velocities for stars of various spectral types and luminosity classes has been determined in this paper, and the location of RS CVn stars as a class is discussed.
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The cosmic origins spectrograph
James C. Green,Cynthia S. Froning,Steve Osterman,Dennis Ebbets,Sara H. Heap,Claus Leitherer,Jeffrey L. Linsky,Blair D. Savage,Kenneth R. Sembach,J. Michael Shull,Oswald H. W. Siegmund,Theodore P. Snow,John R. Spencer,S. Alan Stern,John T. Stocke,Barry Y. Welsh,Stephane Beland,Eric B. Burgh,Charles W. Danforth,Brian A. Keeney,Jason B. McPhate,Steven V. Penton,J. Andrews,K. R. Brownsberger,Jon A. Morse,Erik Wilkinson +25 more
TL;DR: The Cosmic Origins Spectrograph (COS) as discussed by the authors is a moderate-resolution spectrograph with unprecedented sensitivity that was installed into the Hubble Space Telescope (HST) in May 2009, during HST Servicing Mission 4 (STS-125).
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New Mass Loss Measurements from Astrospheric Lyman-alpha Absorption
TL;DR: In this article, mass loss rates are used to assess how wind strength varies with coronal activity and age for solar-like stars, and they find evidence that winds suddenly weaken at a certain activity threshold.
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Measured Mass‐Loss Rates of Solar‐like Stars as a Function of Age and Activity
TL;DR: In this article, the mass loss per unit face area is correlated with X-ray surface flux, and a power-law relation is derived for the solar-like GK dwarfs, showing that the solar wind may have been as much as 1000 times more massive in the distant past.
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The Space Telescope Imaging Spectrograph Design
B. E. Woodgate,Randy A. Kimble,Chuck Bowers,Steven B. Kraemer,Mary Elizabeth Kaiser,Anthony C. Danks,J. F. Grady,J. J. Loiacono,Mark D. Brumfield,Lee Feinberg,Theodore R. Gull,Sara R. Heap,Stephen P. Maran,D. J. Lindler,D. Hood,W. Meyer,C. VanHouten,Vic S. Argabright,S. Franka,Richard L. Bybee,David A. Dorn,M. Bottema,Robert A. Woodruff,David Michika,Joe H. Sullivan,J. C. Hetlinger,C. Ludtke,R. Stocker,Alan W. Delamere,D. Rose,I. Becker,H. Garner,J. G. Timothy,Morley M. Blouke,Charles L. Joseph,George F. Hartig,Richard F. Green,Edward B. Jenkins,Jeffrey L. Linsky,J. B. Hutchings,H. W. Moos,Albert Boggess,Fred L. Roesler,Donna Weistrop +43 more
TL;DR: The Space Telescope Imaging Spectrograph (STIS) instrument was installed on the Hubble Space Telescope (HST) during the second servicing mission, in 1997 February, and four bands cover the wavelength range of 115-1000 nm, with spectral resolving powers between 26 and 200,000 as discussed by the authors.