| Publication |
A Closer Look at Some Gas-phase Depletions in the ISM: Trends for O, Ge, and Kr versus {F}_{* }, f(H2), and Starlight Intensity, Jenkins, Edward B., The Astrophysical Journal, 872, 2019-02-01 00:00:00, 2019ApJ...872...55J||Highly-ionized gas; probing energetic galactic environments, Zech, William F., Ph.D. Thesis, 0, 2010-01-01 00:00:00, 2010PhDT.........1Z||Lifetimes and Oscillator Strengths for Ultraviolet Transitions in Singly Ionized Lead, Heidarian, N.,Irving, R. E.,Ritchey, A. M., The Astrophysical Journal, 808, 2015-08-01 00:00:00, 2015ApJ...808..112H||Oxygen Gas-Phase Abundance Revisited, André, M. K.,Oliveira, C. M.,Howk, J. Christopher, The Astrophysical Journal, 591, 2003-07-01 00:00:00, 2003ApJ...591.1000A||Phosphorus in the diffuse interstellar medium, Lebouteiller, V.,Kuassivi,Ferlet, R., Astronomy and Astrophysics, 443, 2005-11-01 00:00:00, 2005A&A...443..509L||The spectroscopic evolution of the symbiotic-like recurrent nova V407 Cygni during its 2010 outburst. I. The shock and its evolution, Shore, S. N.,Wahlgren, G. M.,Augusteijn, T., Astronomy and Astrophysics, 527, 2011-03-01 00:00:00, 2011A&A...527A..98S||Updated interstellar abundance studies and implications for dust models, Jensen, Adam G., Ph.D. Thesis, 0, 2007-01-01 00:00:00, 2007PhDT.........3J |
