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- Publications
- Influence
New Mass-Loss Measurements from Astrospheric Lyα Absorption
- B. Wood, H. Mueller, G. Zank, J. Linsky, S. Redfield
- Physics
- 17 June 2005
Measurements of stellar mass-loss rates are used to assess how wind strength varies with coronal activity and age for solar-like stars. Mass loss generally increases with activity, but we find… Expand
Measured Mass‐Loss Rates of Solar‐like Stars as a Function of Age and Activity
- B. Wood, H. Mueller, G. Zank, J. Linsky
- Physics
- 25 March 2002
Collisions between the winds of solar-like stars and the local interstellar medium result in a population of hot hydrogen gas surrounding these stars. Absorption from this hot H i can be detected in… Expand
The Structure of the Local Interstellar Medium. IV. Dynamics, Morphology, Physical Properties, and Implications of Cloud-Cloud Interactions*
- S. Redfield, J. Linsky
- Physics
- 27 September 2007
We present an empirical dynamical model of the LISM based on 270 radial velocity measurements for 157 sight lines toward nearby stars. Physical parameter measurements (i.e., temperature, turbulent… Expand
Stellar Lyα Emission Lines in the Hubble Space Telescope Archive: Intrinsic Line Fluxes and Absorption from the Heliosphere and Astrospheres*
- B. Wood, S. Redfield, J. Linsky, H. Mueller, G. Zank
- Physics
- 16 March 2005
We search the Hubble Space Telescope (HST) archive for previously unanalyzed observations of stellar H I Lyα emission lines, our primary purpose being to look for new detections of Lyα absorption… Expand
Deuterium and the Local Interstellar Medium: Properties for the Procyon and Capella Lines of Sight
We present Goddard High-Resolution Spectrograph observations of the interstellar H I and D I Lyct lines and the Mg II and Fen resonance lines formed along the lines of sight toward the nearby stars… Expand
Discovery of a Little Homunculus within the Homunculus Nebula of η Carinae
- K. Ishibashi, K. Ishibashi, +22 authors D. Weistrop
- Physics
- 1 June 2003
We report long-slit spectroscopic mapping of the η Carinae nebula obtained using the Space Telescope Imaging Spectrograph. The observations reveal the presence of a previously unknown bipolar… Expand
The Far-Ultraviolet Spectrum of TW Hydrae. I. Observations of H2 Fluorescence
- G. Herczeg, J. Linsky, J. Valenti, C. Johns-Krull, B. Wood
- Physics
- 18 January 2002
We observed the classical T Tauri star TW Hya with the Space Telescope Imaging Spectrograph on board the Hubble Space Telescope (HST) using the E140M grating, from 1150 to 1700 A, with the E230M… Expand
The On-Orbit Performance of the Space Telescope Imaging Spectrograph
- R. Kimble, B. Woodgate, +87 authors T. Wolfe
- Physics
- 10 January 1998
The Space Telescope Imaging Spectrograph (STIS) was successfully installed into the Hubble Space Telescope (HST) in 1997 February, during the second HST servicing mission, STS-82. STIS is a versatile… Expand
Goddard high-resolution spectrograph observations of the local interstellar medium and the deuterium/hydrogen ratio along the line of sight toward Capella
HST Goddard High-Resolution Spectrograph observations of the 1216, 2600, and 2800 A spectral regions are analyzed for the spectroscopic binary system Capella, obtained at orbital phase 0.26 with… Expand
Atomic deuterium/hydrogen in the Galaxy
- J. Linsky
- Physics
- 3 September 2003
An accurate value of the D/H ratio in the local interstellar medium (LISM) and a better understanding of the D/H variations with position in the Galactic disk and halo are vitally important questions… Expand