The interstellar medium surrounding the Sun
PC Frisch, S Redfield, JD Slavin - Annual Review of Astronomy …, 2011 - annualreviews.org
The Solar System is embedded in a flow of low-density, warm, and partially ionized
interstellar material that has been sampled directly by in situ measurements of interstellar …
interstellar material that has been sampled directly by in situ measurements of interstellar …
A unified representation of gas-phase element depletions in the interstellar medium
EB Jenkins - The Astrophysical Journal, 2009 - iopscience.iop.org
ABSTRACT A study of gas-phase element abundances reported in the literature for 17
different elements sampled over 243 sight lines in the local part of our Galaxy reveals that …
different elements sampled over 243 sight lines in the local part of our Galaxy reveals that …
Three-dimensional extinction maps: Inverting inter-calibrated extinction catalogues
JL Vergely, R Lallement, NLJ Cox - Astronomy & Astrophysics, 2022 - aanda.org
Context. Three-dimensional (3D) maps of the extinction density in the Milky Way can be built
through the inversion of large catalogues of distance-extinction pairs for individual target …
through the inversion of large catalogues of distance-extinction pairs for individual target …
The trouble with the Local Bubble
BY Welsh, RL Shelton - Astrophysics and Space Science, 2009 - Springer
The model of a Local Hot Bubble has been widely accepted as providing a framework that
can explain the ubiquitous presence of the soft X-ray background diffuse emission. We …
can explain the ubiquitous presence of the soft X-ray background diffuse emission. We …
What is the total deuterium abundance in the local galactic disk?
JL Linsky, BT Draine, HW Moos… - The Astrophysical …, 2006 - iopscience.iop.org
Analyses of spectra obtained with the Far Ultraviolet Spectroscopic Explorer (FUSE)
satellite, together with spectra from the Copernicus and interstellar medium absorption …
satellite, together with spectra from the Copernicus and interstellar medium absorption …
The structure of the local interstellar medium. IV. Dynamics, morphology, physical properties, and implications of cloud-cloud interactions
S Redfield, JL Linsky - The Astrophysical Journal, 2008 - iopscience.iop.org
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 …
measurements for 157 sight lines toward nearby stars. Physical parameter measurements …
Project AMIGA: the circumgalactic medium of Andromeda
Project AMIGA: The Circumgalactic Medium of Andromeda - IOPscience This site uses cookies.
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Elemental compositions of two extrasolar rocky planetesimals
S Xu, M Jura, D Koester, B Klein… - The Astrophysical …, 2014 - iopscience.iop.org
We report Keck/HIRES and Hubble Space Telescope/COS spectroscopic studies of
extrasolar rocky planetesimals accreted onto two hydrogen atmosphere white dwarfs, G29 …
extrasolar rocky planetesimals accreted onto two hydrogen atmosphere white dwarfs, G29 …
New 3D gas density maps of NaI and CaII interstellar absorption within 300 pc
BY Welsh, R Lallement, JL Vergely… - Astronomy & …, 2010 - aanda.org
Aims. We present new high resolution (R> 50 000) absorption measurements of the NaI
doublet (5889-5895 Å) along 482 nearby sight-lines, in addition to 807 new measurements …
doublet (5889-5895 Å) along 482 nearby sight-lines, in addition to 807 new measurements …
The accretion-diffusion scenario for metals in cool white dwarfs
D Koester, D Wilken - Astronomy & Astrophysics, 2006 - aanda.org
We calculated diffusion timescales for Ca, Mg, Fe in hydrogen atmosphere white dwarfs with
temperatures between 5000 and 25 000 K. With these timescales we determined accretion …
temperatures between 5000 and 25 000 K. With these timescales we determined accretion …