2003/05/30 by J. T. Lauroesch, David M. Meyer · 30 citations
Physics and Astronomy · #Absorption (acoustics) #Absorption spectroscopy #Astro and Planetary Science #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Galaxy #Hubble space telescope #Interstellar cloud #Interstellar medium #Ion #Ionization #Optics #Physics #Space Telescope Imaging Spectrograph #Spectral line #Spectrograph #Stars #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.1086/377164
published in The Astrophysical Journal 591(2), L123-L126 (IOP Publishing) · 12 pages, 2 figures, accepted for publication in the Astrophysical Journal Letters
arxiv created 2003/05/30 · openalex publication_date 2003/06/13 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
We present multiepoch KPNO coudé feed telescope observations of interstellar Na I and Ca II absorption toward the bright star ρ Leo. Comparisons of the Na I profiles observed over a period of 8 yr reveal significant temporal variations in the Na I column in at least one component, implying that there is "structure" at scales on the order of the proper motion (~12 AU). Archival Hubble Space Telescope ( HST ) Goddard High Resolution Spectrograph observations of the C I fine-structure excitation in the variable component suggest that the density is ≲20 cm -3 , significantly lower than the densities inferred in past H I 21 cm and Na I studies. We suggest that the bulk of the trace neutral species are in the density peaks within an interstellar cloud. The patchy distribution of these species naturally gives rise to the large fluctuations seen on scales of 10-1000 AU in past temporal and binary studies. This picture predicts that the scales over which fluctuations will be observed vary as a function of the ionization rate of a species.