A Reexamination of Phosphorus and Chlorine Depletions in the Diffuse Interstellar Medium
暂无分享,去创建一个
[1] B. Fegley,et al. Solar system abundances and condensation temperatures of the halogens fluorine, chlorine, bromine, and iodine , 2023, Geochemistry.
[2] M. Barlow,et al. The efficiency of grain growth in the diffuse interstellar medium , 2021, Monthly Notices of the Royal Astronomical Society.
[3] Heidelberg,et al. Estimating distances from parallaxes. V: Geometric and photogeometric distances to 1.47 billion stars in Gaia Early Data Release 3. , 2020, 2012.05220.
[4] D. York,et al. HD 62542: Probing the Bare, Dense Core of a Translucent Interstellar Cloud , 2020, The Astrophysical Journal.
[5] S. Federman,et al. Lifetimes and Oscillator Strengths for Ultraviolet Transitions in Neutral Chlorine , 2019, The Astrophysical Journal.
[6] E. Jenkins,et al. A Closer Look at Some Gas-phase Depletions in the ISM: Trends for O, Ge, and Kr versus , f(H2), and Starlight Intensity , 2019, The Astrophysical Journal.
[7] T. Henning,et al. Iron and Silicate Dust Growth in the Galactic Interstellar Medium: Clues from Element Depletions , 2018, 1803.01929.
[8] S. Federman,et al. Abundances and Depletions of Neutron-capture Elements in the Interstellar Medium , 2018, The Astrophysical Journal Supplement Series.
[9] L. Verstraete,et al. The global dust modelling framework THEMIS (The Heterogeneous dust Evolution Model for Interstellar Solids) , 2017, 1703.00775.
[10] S. Bromley,et al. Dust formation in the oxygen-rich AGB star IK Tauri , 2015, 1509.07613.
[11] P. Noterdaeme,et al. Neutral chlorine and molecular hydrogen at high redshift , 2015, 1501.07165.
[12] A. Sarangi,et al. Condensation of dust in the ejecta of Type II-P supernovae , 2014, 1412.5522.
[13] K. Ohnaka,et al. New insights into the dust formation of oxygen-rich AGB stars , 2013, 1310.1924.
[14] A. Hibbert,et al. E1 oscillator strengths and transition rates among levels of Cl I , 2013 .
[15] H. Gail,et al. Seed particle formation for silicate dust condensation by SiO nucleation , 2013, 1305.2879.
[16] U. Sheffield,et al. Interstellar TiII in the Milky Way and Magellanic Clouds , 2010, 1001.3687.
[17] D. York,et al. Molecular Hydrogen in the FUSE Translucent Lines of Sight: The Full Sample , 2008, 0809.3831.
[18] N. Abel,et al. Ultraviolet Survey of CO and H2 in Diffuse Molecular Clouds: The Reflection of Two Photochemistry Regimes in Abundance Relationships , 2008, 0807.0940.
[19] T. Snow,et al. A Study of the ρ Ophiuchi Cloud: Mapping the Distribution and the Motions of Interstellar Gas , 2008 .
[20] A. Jensen,et al. The Variation of Magnesium Depletion with Line-of-Sight Conditions , 2007, 0710.1064.
[21] T. Snow,et al. New Insights on Interstellar Gas-Phase Iron , 2007, 0710.1062.
[22] B. Williams,et al. Spitzer Space Telescope Observations of Kepler’s Supernova Remnant: A Detailed Look at the Circumstellar Dust Component , 2007, astro-ph/0703660.
[23] S. Federman,et al. Oscillator Strengths for Ultraviolet Transitions in P II , 2007, The Astrophysical Journal.
[24] T. Snow,et al. The Abundance of Interstellar Fluorine and Its Implications , 2006, astro-ph/0611066.
[25] S. Friedman,et al. Chlorine in the Galactic ISM: Revised f-values with FUSE and STIS , 2006, astro-ph/0609132.
[26] C. Fischer,et al. Relativistic energy levels, lifetimes, and transition probabilities for the sodium-like to argon-like sequences , 2006 .
[27] D. York,et al. Abundances and Behavior of 12CO, 13CO, and C2 in Translucent Sight Lines , 2006, astro-ph/0608557.
[28] J. Lauroesch,et al. The Homogeneity of Interstellar Elemental Abundances in the Galactic Disk , 2005, astro-ph/0512312.
[29] A. Hibbert,et al. Transitions in Mn ii of astrophysical importance , 2005 .
[30] V. Lebouteiller,et al. Phosphorus in the diffuse interstellar medium , 2005, astro-ph/0507404.
[31] N. D. Gibson,et al. Oscillator Strengths for Ultraviolet Transitions in Cl II and Cl III , 2005 .
[32] V. Smith,et al. Far Ultraviolet Spectroscopic Explorer Measurements of Interstellar Fluorine , 2004, astro-ph/0410362.
[33] K. Gordon,et al. Ultraviolet Extinction Properties in the Milky Way , 2004, astro-ph/0408409.
[34] D. Morton,et al. Atomic Data for Resonance Absorption Lines. III. Wavelengths Longward of the Lyman Limit for the Elements Hydrogen to Gallium , 2003 .
[35] J. Lauroesch,et al. The Homogeneity of Interstellar Oxygen in the Galactic Disk , 2003, astro-ph/0406385.
[36] K. Lodders. Solar System Abundances and Condensation Temperatures of the Elements , 2003 .
[37] S. Tayal. Oscillator Strengths of Allowed and Intercombination Lines in P II , 2003 .
[38] D. York,et al. A FUSE Survey of Interstellar Molecular Hydrogen in Translucent Clouds , 2002, astro-ph/0205415.
[39] D. York,et al. Abundances and Physical Conditions in the Interstellar Gas toward HD 192639 , 2002, astro-ph/0205403.
[40] J. Lauroesch,et al. Space Telescope Imaging Spectrograph Observations of Interstellar Oxygen and Krypton in Translucent Clouds , 2001 .
[41] D. York,et al. A Far Ultraviolet Spectroscopic Explorer Survey of Interstellar Molecular Hydrogen in the Small and Large Magellanic Clouds , 2001, astro-ph/0110262.
[42] J. Weingartner,et al. Interstellar Depletion onto Very Small Dust Grains , 1998, astro-ph/9812469.
[43] D. Welty,et al. A High-Resolution Survey of Interstellar K I Absorption , 1996 .
[44] A. Tielens,et al. Grain destruction in shocks in the interstellar medium , 1994 .
[45] S. Federman,et al. Accurate oscillator strengths for interstellar ultraviolet lines of Cl I , 1993 .
[46] B. Savage,et al. The analysis of apparent optical depth profiles for interstellar absorption lines , 1991 .
[47] J. Black,et al. The photodissociation and chemistry of interstellar CO , 1988 .
[48] A. Hibbert. Transitions in P II , 1988 .
[49] B. Savage,et al. Abundances of interstellar atoms from ultaviolet absorption lines , 1986 .
[50] A. Harris,et al. The abundance of interstellar chlorine in the galaxy , 1984 .
[51] Ralph C. Bohlin,et al. A survey of ultraviolet interstellar absorption lines , 1983 .
[52] D. York,et al. The detection of interstellar fluorine in the line of sight toward Delta Scorpii , 1981 .
[53] E. Dwek,et al. The evolution of refractory interstellar grains in the solar neighborhood , 1980 .
[54] B. Savage,et al. A survey of interstellar H I from L-alpha absorption measurements. II , 1978 .
[55] D. York,et al. Observations of interstellar chlorine and phosphorus , 1978 .
[56] R. C. Bohlin,et al. A survey of interstellar molecular hydrogen. I , 1977 .
[57] M. Jura. Chlorine-bearing molecules in interstellar clouds , 1974 .
[58] L. Hobbs. On Ionization in H i Regions , 1974 .